The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light profile. Its shape is moderately elongated, appearing somewhere between round and cigar-shaped. There is a notable lack of distinct spiral arms or a prominent disk-like structure. The color is generally bluish, with a bright center suggesting the presence of older stars. There are some hints of minor disturbances, such as small asymmetries or irregularities in the outer regions of the galaxy, which could suggest that a minor merger or tidal interaction may be occurring. Overall, the galaxy seems relatively isolated, with no obvious major merging activity visible.
