The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity extending outwards from the core. The color appears to be a somewhat muted blue-green, suggesting the presence of a moderate population of relatively young, hot stars, though the overall stellar population is likely dominated by older, redder stars, giving it a slightly yellowish cast. No distinct spiral arms or prominent dust lanes are discernible in this image. There is a very faint suggestion of some minor asymmetry or disturbance to the shape. It does not appear to be undergoing a major merger. Overall, the galaxy's morphology is indicative of an evolved system, possibly undergoing slow, ongoing star formation.
