The galaxy presents as an elliptical morphology, with a moderately flattened shape. Its core exhibits a bright, concentrated luminosity profile, suggesting a high density of stars in the central region. Moving outwards from the core, the luminosity gradually decreases, forming a diffuse halo. The color distribution reveals a predominantly yellow-white hue in the central bulge, indicative of an older stellar population. Fainter blue tinges are observed in the outer regions, possibly indicating the presence of younger stars, or regions of more recent star formation. There is no clear indication of spiral arms or a distinct disk structure, supporting the classification as an elliptical galaxy.
