The galaxy appears as a diffuse, centrally concentrated object. Its overall morphology is somewhat amorphous, lacking clear spiral arms or a well-defined elliptical shape. The central region exhibits a slightly brighter luminosity, suggestive of a galactic nucleus or a higher density of stars. A faint, extended halo surrounds the central region, gradually fading into the background sky.

The color profile indicates a generally older stellar population, with a moderate red hue dominating the overall appearance. There are subtle variations in color within the galaxy, possibly indicating regions of differing star formation activity or dust content. No prominent dust lanes are observed.

There are hints of minor disturbances in the overall shape, possibly due to a past interaction or merger event. A subtle asymmetry is observed in the halo region. However, the image does not clearly show evidence of strong tidal tails or other clear merger signatures. Some features may be present that could be either background noise or artifacts. More data is needed to confirm the existence of certain features.
