The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish hue, suggesting a population of older stars. Moving outwards from the core, the color transitions to a bluer shade, implying the presence of some younger stellar populations, although they appear to be subdued. The galaxy lacks any obvious spiral arm structures or prominent dust lanes. There is no evidence of major ongoing mergers or significant tidal disturbances. The overall light distribution suggests a relaxed system. The shape can be described as being between round and elongated.
