The galaxy presents as a centrally concentrated object with a smooth light distribution. The core exhibits a bright, yellowish hue, suggesting a population of older stars. Extending outward from the core, a fainter, more diffuse envelope is visible, with some subtle bluer regions hinting at possible regions of younger stellar populations. The overall shape appears roughly elliptical, but there is an indication of a faint tidal feature or arm extending from the main body, suggesting a possible interaction or past merger event. Based on the color distribution, star formation activity appears to be low, with the majority of the light emanating from an older stellar population.
