The galaxy presents as an elliptical morphology, exhibiting a relatively smooth light distribution. The isophotes appear elongated, indicating a moderate degree of ellipticity. There is a discernible color gradient, with the central region exhibiting a yellower hue, suggesting a higher concentration of older stellar populations. The outer regions display a bluer tint, which could be indicative of younger stars or ongoing star formation, albeit at a lower rate. There are no apparent signs of spiral arms or significant dust lanes. The overall structure appears undisturbed, lacking tidal features or strong signs of recent merger activity. The galaxy seems to be a fairly massive system with a substantial stellar population.
