The galaxy presents as a centrally concentrated object with a largely smooth, diffuse appearance. It exhibits a generally elliptical morphology, appearing quite round. There is no clear evidence of spiral arms or a defined disk structure at this resolution. The color gradient suggests an older stellar population, concentrated towards the core, with a redder hue in the central region that fades toward the outskirts. Some slightly bluer tints in the outer regions might suggest some ongoing, albeit low-level, star formation activity. No major disturbances or tidal features are obviously visible, implying that it is not actively undergoing a major merger event at this time, though the possibility of a past minor interaction cannot be ruled out. The galaxy is relatively compact in angular size.
