The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a smooth, centrally concentrated morphology. It has a generally round shape with no obvious spiral arm structures or prominent dust lanes visible. The light profile suggests a gradual decrease in brightness outwards from the core. The color index (G-R, R-Z) indicates the stellar population is moderately evolved, which is consistent with a relatively low star formation rate. There is a distinct yellow hue, indicating a population dominated by older stars. Minor disturbance is possible as the galaxy has some visual asymmetry. Overall, this galaxy appears to be a massive elliptical or lenticular galaxy, that is likely to have a supermassive black hole at its center.
