The galaxy presents as a relatively smooth, elliptical morphology. Its color profile suggests a dominant population of older stars, exhibiting a yellowish hue in the central region, which diffuses outward. There is little to no discernible evidence of spiral arms or prominent dust lanes. The overall structure appears largely undisturbed, showing no immediate signs of major mergers or tidal interactions. The galaxy appears fairly round, with only a slight deviation from perfect circularity. The light is concentrated towards the core, indicative of a high stellar density in the nucleus. The galaxy appears to be relatively isolated in its immediate vicinity.
