The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly circular morphology, deviating minimally from a perfect sphere. The color profile suggests a dominant population of older stars, with a yellowish hue indicative of a lack of significant ongoing star formation. There is no readily apparent disk structure or spiral arm features; the galaxy appears largely featureless at this resolution. Subtle irregularities along the edges of the galaxy could indicate minor gravitational interactions, but the overall structure remains largely undisturbed. The galaxy is moderately luminous, suggesting a considerable stellar mass, which is consistent with the observed morphology of an evolved system.
