The galaxy presents a generally smooth and elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity outwards from the core. The central region exhibits a yellowish hue, suggesting an older stellar population. No distinct spiral arms or bar structures are discernible. The galaxy appears largely undisturbed, showing no obvious signs of major mergers or tidal interactions. The shape is somewhat elongated, falling somewhere between round and cigar-shaped. There may be some minor structural irregularities, but the overall appearance is that of a relatively evolved system, with minimal ongoing star formation.
