The galaxy presents as a centrally concentrated, smooth light distribution. The morphology appears largely spheroidal, lacking prominent spiral arms or a distinct disk structure. The light profile exhibits a relatively gradual decline in intensity from the core outwards, suggesting a lack of significant ongoing star formation within the visible region. A yellow-orange hue dominates the galaxy's color, which potentially suggests a population of older stars, consistent with a relatively low star formation rate. No obvious signs of tidal disruption or interaction with other galaxies are observed; it exhibits a fairly relaxed morphology. The roundness also indicates that the galaxy could be an elliptical galaxy viewed face-on or a spiral galaxy viewed directly.
