The galaxy presents a generally elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggestive of a dense stellar population. The luminosity gradually decreases outwards from the center of the galaxy, without any discernible spiral arm structures or prominent dust lanes.

The color gradient across the galaxy seems relatively uniform, with a yellowish hue dominating the visual appearance. This suggests a population of older stars and a low rate of ongoing star formation. There is a slight elongation observed in its shape, but it does not resemble a highly flattened disk. This overall morphology leads to the classification of the galaxy being a smooth elliptical galaxy. There are no indications of major tidal disturbances or ongoing mergers.
