The galaxy presents a generally smooth morphology, appearing largely featureless. The light distribution is centrally concentrated, displaying a bright, yellowish core that likely indicates an older stellar population. Surrounding the core is a more diffuse halo with a bluer hue, suggesting the presence of younger, hotter stars or ongoing star formation, albeit at a seemingly low rate. The galaxy's overall shape appears to be approximately elliptical, with a high degree of roundness. There is no evidence of any major mergers or significant tidal disturbances in this image, though a possible slight asymmetry in the outer regions cannot be completely ruled out.
