The galaxy presents as a centrally concentrated system with a primarily smooth morphology. A distinct bulge component is visible, appearing bright and relatively symmetrical. The outer regions of the galaxy exhibit a more diffuse appearance with a faint disk-like structure. The disk structure is not well-defined, it appears blurred and lacking in prominent spiral arms or other detailed features. There is a slight elongation in the overall shape, though the galaxy tends towards being round, but there is a slightly cigar-like shape. The color profile indicates a generally older stellar population, with a relatively low rate of ongoing star formation. Evidences do not indicate significant interaction, disturbance, or recent merger events.