The galaxy presents a generally smooth, elliptical morphology. It is centrally concentrated with a diffuse halo, exhibiting a somewhat rounded appearance rather than a distinctly flattened or elongated shape. There's a subtle hint of a disk-like structure. The color profile appears relatively uniform across the galaxy, suggesting a lack of significant ongoing star formation within. There is no obvious presence of spiral arms or prominent dust lanes, further supporting the smooth classification. Faint disturbances and a potential minor merger cannot be excluded. The galaxy's overall appearance indicates that it is a relatively evolved system, likely dominated by an older stellar population.
