The galaxy presents a slightly elongated, cigar-shaped morphology. Its light profile appears relatively smooth and centrally concentrated, suggesting a dominant spheroid component. There's an indication of a possible minor interaction or tidal disturbance on one side, with what appears to be a faint extension or plume. The galaxy exhibits a redder color, which could indicate a population of older stars and a lower ongoing star formation rate. There may be a possible merging event occuring with a neighboring object.
