The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, with light gradually fading towards the outer edges. The color profile is dominated by yellowish hues, suggesting an older stellar population with a dearth of ongoing, high-mass star formation. There is little to no visible dust or spiral arm structure discernible in this image. The overall morphology indicates a system that is dynamically relaxed, without any obvious signs of recent mergers or significant tidal disturbances. The object's round shape suggests that it is likely viewed close to face-on.
