The galaxy presents as a centrally concentrated, smooth object with a largely elliptical morphology. The light distribution appears relatively uniform across its structure, with a gradual decrease in intensity moving outward from the core. There is a prominent central bulge exhibiting a yellowish hue, suggesting an older stellar population with minimal ongoing star formation within this region. Faint, slightly bluer extensions are observed along the periphery of the galaxy, potentially indicative of a small amount of recent star formation, or residual disk like feature. Overall, the galaxy's morphology suggests a likely classification as an early-type galaxy, possibly an elliptical or lenticular galaxy with a relatively high degree of spheroidal symmetry. There is no apparent evidence of a strong tidal interaction or major merger event currently affecting the galaxy.
