This galaxy exhibits an overall smooth morphology, characterized by a central bulge that appears approximately round with only a slight ellipticity. The light is concentrated at the center of the galaxy, gradually decreasing towards the edges. There is no obvious spiral arm structure or prominent dust lanes visible in this image. The overall color suggests that this galaxy is relatively old, with a population of evolved stars contributing to the dominant redder wavelengths. There is no significant star formation apparent within the body of the galaxy. It appears undisturbed with no signs of tidal features, major asymmetries, or indications of ongoing merger activity.
