The observed galaxy presents as a relatively compact, though somewhat diffuse, object with a notable reddish-orange hue. The light distribution appears centrally concentrated, indicative of a substantial bulge component. There is some observed asymmetry, with a suggestion of tidal features. This could be indicative of a gravitational interaction or merger event. The overall morphology is mostly smooth, with no prominent spiral arms or distinct dust lanes easily discernible in this image. The color suggests an older stellar population with relatively little ongoing star formation.
