The galaxy appears to be a relatively smooth, rounded object with a concentrated central bulge. Its color profile suggests an older stellar population dominating the bulge, indicated by the yellowish-orange hue. The surrounding regions exhibit a bluer tint, hinting at the presence of younger, hotter stars and potential ongoing star formation, though at a low rate. There is no obvious spiral structure or prominent dust lanes visible in this image, suggesting it might be an elliptical galaxy, or possibly a lenticular galaxy seen face-on with a faint disk. There is no obvious distortion or tidal features indicative of recent or ongoing major merger activity, although minor disturbances are possible. The galaxy has an estimated size of around 6 kiloparsecs, making it a moderate sized galaxy. The overall morphology indicates a relatively evolved system with a moderate mass and a moderate absolute magnitude.
