The galaxy presents a generally elliptical morphology, with a relatively smooth light distribution and a high degree of central concentration. The dominant color is a warm, yellowish hue, indicating a population of older stars. A subtle reddish tint is visible in the central regions, possibly indicative of dust or more evolved stellar populations. No prominent spiral arm structure or distinct features are visible. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or ongoing mergers. There may be a slight elongation.
