This galaxy exhibits a morphology consistent with an elliptical galaxy, characterized by a smooth, elongated shape. The central bulge is bright and concentrated, displaying a yellowish hue, suggestive of an older stellar population. Extending outwards from the core, the galaxy appears to have a faint, diffuse halo with a bluish tint at the edges. The notable ellipticity suggests a significant amount of angular momentum may be present, potentially influencing the distribution of stars and dust within the galaxy. There appears to be little or no evidence of spiral arm structures or prominent dust lanes. This galaxy seems to be in a relatively quiescent state regarding star formation activity, which is expected for its morphological classification.
