The galaxy presents as a relatively smooth object with a generally elliptical morphology. The central region exhibits a concentrated luminosity profile, appearing brighter and more yellowish, possibly indicative of an older stellar population. Moving outwards from the core, the galaxy fades into a diffuse halo or disk structure. The shape appears elongated or cigar-shaped, suggesting that it may be an elliptical galaxy viewed at an angle or possibly a lenticular galaxy with a subtle disk component. The presence of some bluer hues along the outer regions hints at a small amount of ongoing star formation. No significant tidal features or nearby companions are visible. Overall, the galaxy appears relatively undisturbed, with no signs of major merging events in its recent history.
