The galaxy appears as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge that diminishes gradually outward, lacking any discernible spiral arm features in this observation. The galaxy's color profile seems to be largely homogenous, with a yellow to golden hue that would suggest older stellar populations, and that is indicative of a galaxy with decreased star formation. The shape of the galaxy is generally rounded. A very slight asymmetry might be present, though it is difficult to discern from this image. No significant interactions or tidal features are immediately obvious, suggesting it is likely a relatively isolated system that is not undergoing any major mergers.
