The galaxy presents as a single, relatively smooth object with a somewhat elliptical shape. The color profile suggests a dominant population of older stars, with the core exhibiting a strong yellowish hue indicative of an evolved stellar population. The overall structure indicates that it is likely an early-type galaxy, or a spiral galaxy viewed at an angle. Some minor disturbances may be occurring based on the slight distortion of the overall shape, although further investigation into the presence of tidal tails or other merger signatures is needed to confirm this. There are no visible spiral arms or prominent dust lanes apparent in this image. The star formation rate is also notably low.
