The galaxy presents as a relatively smooth, elliptical morphology. A pronounced central bulge is observed, exhibiting a yellowish-white hue, suggesting a population of older stars. Moving outward from the bulge, the galaxy displays a faint, diffuse disk structure that exhibits blue tinges. These likely signify areas of more recent star formation, albeit at a moderate rate relative to the overall mass of the galaxy. The object appears elongated. There is no evidence of significant tidal features or ongoing major mergers; minor disturbances may exist. The galaxy appears to be isolated, with no other large objects in proximity.
