The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth luminosity profile. The central region exhibits a bright, yellowish hue, suggesting a population of older stars. Moving outward from the core, the color gradient shifts towards a redder tone, which also suggests an aging stellar population. There is very little evidence of spiral arm structure or significant dust lanes. The overall morphology indicates a mature galaxy with a low rate of current star formation. There may be a slight asymmetry, but no apparent major tidal features or signs of ongoing merger activity are visible.
