The galaxy presents an overall elliptical morphology, with a smooth, centrally concentrated luminosity profile indicative of a bulge component. Faint disc-like features are present, appearing as an extended structure. The color suggests an older stellar population, with a noticeable lack of blue light, potentially indicating a lower rate of ongoing star formation. There is no evidence of any major mergers or tidal disruptions, although slight asymmetries in the outer regions cannot be entirely ruled out without further analysis. The object is oriented with its major axis tilted, offering a moderately inclined view of the galaxy's structure.
