The galaxy appears to be a relatively compact object, characterized by a smooth, elliptical morphology. The light distribution suggests a high degree of central concentration, with brightness decreasing radially outwards from the core. No distinct spiral arms or bar structures are discernible. The color profile is suggestive of a mature stellar population, with a yellowish-white hue dominating the central region, possibly indicative of older, redder stars. There's a slight hint of bluer light at the edges of the galaxy. There is no sign of any on going mergers or major disturbances.
