The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, exhibiting a gradual falloff in intensity with increasing radius. The color is predominantly yellow-orange, suggesting a stellar population that is relatively old. The galaxy appears fairly undisturbed, lacking obvious signs of recent major mergers or tidal interactions. There is little evidence of distinct spiral arms or a prominent disk structure, consistent with a classification towards the elliptical end of the Hubble sequence. Subtle colour variations may indicate underlying substructure or variations in stellar populations within the galaxy. The object exhibits a relatively round shape. There is no obvious presence of a strong central bar or ring-like feature.
