The galaxy appears to be a relatively bright object with a somewhat smooth morphology. The light distribution suggests it is centrally concentrated, exhibiting a rounded shape instead of a distinctly elongated or irregular form. There isn't an immediately obvious disk structure; instead, the light seems to fade gradually from the center outwards, indicating a significant bulge component. There are possible signs of some tidal activity, perhaps due to recent minor disturbances or interactions, but is overwhelmingly of a non-merging classification. The colours suggest a stellar population with a range of ages. Overall, this galaxy presents as a galaxy with a considerable spheroidal component, with some indication of weak ongoing or recent activity.
