The galaxy presents a generally smooth, elliptical morphology. The central region appears to be highly concentrated and bright, with a yellowish hue, suggesting an older stellar population. The outer regions show a gradual decrease in surface brightness with no distinct spiral arm structures or prominent dust lanes visible. There is a slight elongation, but overall the galaxy appears nearly round in shape. No signs of major mergers or tidal disturbances are apparent from this image. The galaxy exhibits a red shift of 0.260646. Based on these properties, this galaxy is consistent with being a massive elliptical galaxy with a relatively low ongoing star formation rate.
