The galaxy presents a predominantly smooth and round morphology. The color profile indicates a concentrated yellowish-orange core, suggesting a population of older stars. There's a subtle, diffuse halo surrounding the core that extends outwards, exhibiting a gradual color shift towards redder hues, implying a slightly older stellar population in the outer regions. No spiral arm structures or significant dust lanes are discernible within the observed image, further supporting the interpretation of a relatively featureless elliptical-like or lenticular galaxy. There is no evidence of major mergers or significant tidal disturbances in the image.
