The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The core region exhibits a bright, diffuse glow, suggesting a significant population of older stars. A subtle color gradient is observed, transitioning from a slightly bluer hue in the outer regions to a redder hue towards the core. There are no readily apparent spiral arms or distinct dust lanes. The general form is generally round, exhibiting no signs of significant tidal disruption or interaction with other galaxies. Subtle irregularities at the edge suggest a smooth transition into the intergalactic medium.
