The galaxy appears as a concentrated, centrally luminous object, exhibiting a generally smooth morphology. The primary light distribution is concentrated in a bright, yellow-white core, suggesting a significant population of older stars. The overall shape is largely elliptical with a smooth, diffuse outer region characterized by a faint, extended halo. There is no apparent spiral structure or prominent dust lanes visible. A lack of significant color variations suggests a relatively uniform stellar population throughout the galaxy. No evidence of tidal features or ongoing major mergers is observed.
