The galaxy appears to be a relatively smooth, early-type system, likely an elliptical. The light profile exhibits a centrally concentrated bulge with a gradual decrease in intensity outward, suggesting an older stellar population. There is a slight elongation, indicating it is not perfectly spherical, with a subtle cigar shape. There is no distinct spiral structure or prominent dust lanes visible. No major merger or tidal disturbances are apparent in the image. The galaxy presents a moderate luminosity, with an overall red color index compared to the g band. This suggests that the star formation activity is relatively low. The galaxy has a medium stellar mass.