The galaxy presents as a relatively smooth, centrally concentrated object. The light profile suggests a dominant spheroidal component. The color is yellowish-white, potentially indicating a population of older stars and a relatively low rate of ongoing star formation. There's a subtle suggestion of a slight extension or elongation, but the galaxy is generally round in appearance. There is no clear evidence of a distinct disk component, spiral arms, or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed, not currently undergoing a major merger event.
