The galaxy presents a smooth, elliptical morphology with a dominant, spheroidal component. It appears as a relatively compact object, with no readily discernible spiral arms or other disk-like features. The galaxy exhibits a pronounced color gradient, transitioning from a yellowish core to a bluer outer region. The core is bright and concentrated, suggesting a significant population of older stars, while the bluer halo may indicate more recent star formation activity or the presence of a younger stellar population. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. The object appears fairly isolated and relaxed, without clear signs of interaction with neighboring galaxies.
