The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. There is a subtle flattening of the disk, giving it a slightly oval appearance. The light distribution appears brightest and most concentrated towards the center, gradually fading outwards. The overall color appears yellowish-white, indicating an older stellar population. There is little evidence of significant dust lanes or spiral arm structures. The galaxy does not appear to be undergoing any major merger events, though minor disturbances cannot be ruled out.