The galaxy appears as a single, centrally concentrated object. It exhibits a largely smooth morphology, with a dominant spheroidal component and minimal discernible disk features. Coloration suggests a relatively evolved stellar population, with a central concentration of redder hues, possibly indicating older stars. There appears to be ongoing, if subdued, star formation within the galaxy, noted by the presence of blue light. No major mergers or disturbances are readily apparent in the image, though there is an observed minor disturbance. The galaxy has a moderately luminous profile. The galaxy appears fairly rounded, without a strongly elongated or irregular shape.
