The object appears to be a galaxy, exhibiting a generally smooth morphology with a dominant spheroidal component. Its color profile suggests a moderate population of older stars, contributing to the overall yellowish-orange hue. There may be a faint, diffuse disk surrounding the central bulge, although this is not definitive. The galaxy is relatively isolated, showing no obvious signs of recent major mergers, though some minor distortions might be present. The shape is primarily round, with minimal elongation. Overall, this galaxy appears to be a relatively evolved system, with ongoing, but limited star formation activity.
