The galaxy exhibits a moderately elongated morphology. A relatively smooth overall appearance is observed, with the central bulge appearing more prominent than the surrounding disk. The color gradient transitions from a bluer hue in the outer regions to a yellower, potentially older stellar population concentrated in the central bulge. There is evidence of possible minor disturbances in the structure, such as faint tidal features or asymmetries that hint at past or ongoing interactions. Star formation activity appears to be relatively low overall, inferred from the redder colors and lack of prominent blue star-forming regions. The system may possibly be composed of two galaxies, where one is smaller than the other.
