The galaxy presents a predominantly smooth morphology, suggesting a classification as an elliptical galaxy. The core region is highly luminous, with a yellowish-white hue indicating a high concentration of older stellar populations. The galaxy exhibits a radial decrease in surface brightness from the core outwards, with a gradual transition to a fainter, more diffuse halo. The shape appears close to circular, with a slight elongation. There is no clear evidence of spiral arms, dust lanes, or other distinct features typically associated with spiral galaxies. The overall color is consistent with a relatively passive galaxy with low ongoing star formation. There are hints of possible minor tidal disturbances and/or a faint disc, but there is no definitive evidence of an ongoing major merger.
