The galaxy appears to be undergoing a significant interaction, possibly a merger. It is not a simple elliptical or spiral; it shows a disturbed morphology, with a main central body and a region of lower surface brightness extending from the central region. There are signs of tidal tails or streams, indicating gravitational disruption. The main body exhibits a slightly yellowish hue, suggesting a population of older stars or a moderate level of dust extinction. Patches of bluer light are present, possibly indicating ongoing star formation. The overall structure is somewhat irregular, lacking a well-defined spiral arm structure or a smooth elliptical profile. The galaxy appears relatively large, subtending a considerable angular size. Based on its overall appearance, it seems likely to be a relatively massive system with ongoing or recent star formation.
