The galaxy presents an elliptical morphology, appearing largely smooth and somewhat rounded in shape. A bright, concentrated central bulge is evident, surrounded by a fainter, more diffuse halo. There is a subtle disk component, exhibiting some faint features. Some minor disturbances are apparent, though no major merger activity is indicated based on the image. Color gradients suggest a diverse stellar population, potentially indicating moderate star formation is occurring. The galaxy exhibits a notable luminosity, suggesting a relatively high stellar mass. Overall, the galaxy appears to be a moderately massive system with a relatively old stellar population and some ongoing star formation.
