The galaxy presents a largely elliptical morphology with a smooth, diffuse appearance, with an overall yellow to orange hue concentrated in the central region, likely indicating an older stellar population. There is very little evidence of spiral arm structure or significant dust lanes from the image. The light distribution suggests a generally spheroidal shape, with a fairly high degree of central concentration. The edges fade gradually into the background, lacking sharp definition. There is a slight indication of a faint, extended halo surrounding the main body of the galaxy, exhibiting a bluer tint compared to the core, which could signify traces of on-going star formation. The galaxy appears relatively undisturbed, with no obvious signs of major merging activity or tidal distortions. However, there is a slight asymmetry, with the upper region showing a subtle extension.
