The galaxy appears as a smooth, elliptical structure with a moderately concentrated central bulge. Its overall shape is elongated, leaning towards a cigar-like form, but not extremely so. The color distribution suggests an older stellar population, with a yellowish hue dominating, indicating lower levels of ongoing star formation. There is no obvious evidence of spiral arms or significant dust lanes. No major mergers or disturbances are apparent in its morphology; any potential minor disturbance would be difficult to detect given the image resolution. The galaxy appears relatively isolated and is not currently interacting with a companion galaxy.
