This galaxy exhibits a generally smooth morphology, with an overall elliptical shape. It does not appear to have prominent spiral arms or a well-defined disk structure. The light distribution is concentrated towards the center, exhibiting a bulge that appears reddish in color, potentially indicating an older stellar population. Surrounding the bulge is a somewhat diffuse, greenish halo, which could be indicative of a mix of stellar populations or ongoing star formation at a low rate. There is no obvious evidence of tidal features, ongoing mergers, or significant dust lanes within the galaxy. The galaxy appears relatively undisturbed and isolated.
