The galaxy presents as a centrally concentrated object with a relatively smooth appearance. There is a dominant, bright central bulge that is slightly oblong. The overall shape is neither perfectly round nor highly elongated. The light distribution gradually fades from the core outwards, suggesting a lack of distinct spiral arms or prominent features. The color appears to be a yellowish-white, potentially indicating an older stellar population within the bulge. There are no apparent signs of a major ongoing merger, though a subtle asymmetry cannot be completely ruled out. The disk appears indistinct with no clear dust lanes or prominent star-forming regions.
