The galaxy presents as a generally smooth, elliptical-like object. The central region exhibits a high degree of light concentration, appearing significantly brighter and more yellow than the outer regions. The light gradually diffuses outward from the center, fading into a redder hue at the edges. There is no obvious spiral arm structure, and the overall morphology suggests a relatively evolved system with little ongoing major star formation. A slight asymmetry hints at a possible minor interaction, but no clear tidal features or strong disturbances are evident. The galaxy appears moderately massive, potentially a transition object between spiral and elliptical types.
