The galaxy exhibits a generally smooth morphology, though some features are discernible. Its shape is elongated, approaching a cigar-like form. The color distribution suggests a dominant population of older stars, with a noticeable reddish hue concentrated towards the central region. There is a slight indication of bluer light possibly associated with younger stars within a disk-like structure. However, the smoothness of the galaxy implies that it could be a smooth galaxy that may be on the verge of becoming a elliptical one, not actively forming stars at a high rate. There is no apparent evidence of a major merger or significant tidal disturbance. Overall, this galaxy appears to be a quiescent, relatively massive system.
