The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is yellowish in color, suggesting an older stellar population. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears somewhat round in shape, with a slight elongation. No major merger events or tidal disturbances are readily apparent, although there is potentially some minor disruption in the halo. Overall, the galaxy appears to be a relatively quiescent system.