The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a yellowish-white hue, suggesting an older stellar population. The isophotes appear elongated, with an approximate aspect ratio of 2:1. The outer regions of the galaxy display a bluer tint, possibly indicating the presence of younger stars or ongoing star formation, although the smooth texture suggests this is not a spiral galaxy. No distinct features such as spiral arms, bars, or dust lanes are readily apparent. There is no evidence of a major merger in progress or tidal features resulting from interactions. Overall, the galaxy appears to be a relatively isolated, moderately luminous, and relatively massive system at a moderate redshift.
