The galaxy presents a predominantly smooth, elliptical morphology. The central region exhibits a high concentration of light, suggestive of a bulge component. Moving outward, the light intensity gradually decreases, transitioning into a less defined halo.

There is evidence of a slight disk-like structure or arm features within the galaxy. A subtle, bluer-tinged area is visible on the right side, possibly indicating a region of more active star formation. However, these features are not sharply defined, suggesting a more diffuse and less structured spiral pattern.

Overall, the galaxy appears as a transition between a pure elliptical and a spiral galaxy, potentially an early-type spiral or a lenticular galaxy with subtle spiral features. No major merger events or tidal disruptions are apparent.
