The galaxy exhibits a distinct elliptical morphology, appearing elongated with a cigar-like shape. It displays a smooth, featureless profile, lacking prominent spiral arms or a well-defined disk structure. The galaxy's color gradient transitions from a more reddish hue in the central region to a slightly bluer color towards its outer edges. This color variation suggests a stellar population gradient, with older, redder stars concentrated in the core and younger, bluer stars more prevalent in the outskirts. The light distribution is relatively even, with a gradual decrease in brightness from the center outwards, consistent with a low specific star formation rate. There is no evidence of significant tidal disturbances or ongoing merging activity based on the galaxy's overall structure, although there is a possibility of a minor interaction having taken place in its past.
