The galaxy presents as a slightly elongated structure with a generally smooth appearance. The overall color profile suggests a population of older stars, indicated by a dominant reddish hue in the central region. The galaxy exhibits a slight deviation from perfect sphericity, appearing somewhat elliptical. There is evidence of a potential minor disturbance or interaction, indicated by a subtle asymmetry in the galactic structure, possibly a faint tidal tail or uneven distribution of light. There are indications of recent or ongoing star formation, evidenced by a weak blue tint dispersed sparsely throughout the body.
