The galaxy presents as a largely featureless, elliptical-type system. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish hue. The light profile appears smooth and relatively undisturbed. There is little to no evidence of spiral arm structure or significant dust lanes. The overall morphology suggests a galaxy in which star formation activity has slowed, leading to an older stellar population, particularly within the central bulge. A very faint red tint is visible in the outer regions of the galaxy, though whether this is a stellar population or dust feature is unclear. The system is moderately luminous, indicating a substantial stellar mass.