The galaxy presents as an elliptical morphology, with a smooth, diffuse appearance, consistent with an early-type galaxy. It exhibits a concentrated central bulge with a gradual decline in surface brightness towards the outer regions. The primary color is a yellowish-white hue, suggesting an older stellar population with fewer young, massive stars. There appears to be very little evidence of spiral arm structure or dust lanes, further indicating a lack of ongoing significant star formation. The shape is generally round, with an axial ratio close to unity, though with a slight elongation. There are no immediately apparent signs of tidal disturbances or ongoing mergers, although subtle asymmetries cannot be entirely ruled out at this resolution.
