The galaxy presents a roughly elliptical morphology, exhibiting a smooth, diffuse appearance, with no discernible spiral arm structure or prominent dust lanes. The central region appears brighter and more concentrated, suggesting a possible bulge. The galaxy's color profile indicates a redder hue in the central region, transitioning to a slightly bluer color towards the outer edges. There may be some evidence of minor tidal disturbances or interactions, indicated by the subtle asymmetry in the outer regions. Overall, the galaxy appears to be a relatively massive system with moderate ongoing star formation activity. It may be an early-type spiral or an elliptical galaxy undergoing some interaction.
