The galaxy presents as a slightly elongated, disk-shaped object. It appears to possess a prominent bulge, characterized by a concentrated, bright central region exhibiting a yellowish-white hue. The disk component shows a fainter luminosity relative to the bulge. Hints of spiral arm structures are not distinctly discernable. The overall color suggests the presence of a relatively older stellar population. The morphology leans towards a smooth and undisturbed structure, with no clear signs of ongoing major mergers. The shape suggests an oblate spheroid with a slight cigar shape. There is only very minor disturbance visible. Star formation appears low overall.
