The galaxy presents as a luminous, centrally concentrated object with a largely smooth morphology. The overall shape appears roughly elliptical or spheroidal, with a high degree of circularity. There is a concentration of light towards the center of the object, suggesting a bulge or core component. The radial light profile diminishes gradually from the core outwards, without any distinct breaks or sharp features.

The galaxy's color is distinctly redder in comparison to other celestial objects in the field, potentially indicating an older stellar population, significant dust extinction, or a high redshift. While largely smooth, there might be some subtle features indicative of minor disturbances in the galaxy's outer regions, such as faint tidal tails or asymmetries, though these are not prominent. There are no well-defined spiral arms or bar structures discernible in the image. A small portion of the object appears to be merging with something. The galaxy does have an apparent size to the scale.
