The galaxy exhibits a primarily elliptical morphology, appearing as a smooth, concentrated luminosity profile with a notable absence of distinct spiral arms or prominent dust lanes. It has an intermediate apparent ellipticity, suggesting a shape between spherical and elongated. The central region displays a bright, concentrated core, possibly indicative of a supermassive black hole or a dense stellar population. Colors are generally uniform, with a slightly reddish or yellowish hue indicating a population of older stars. The overall appearance implies a relatively evolved galaxy with a low rate of active star formation. There is little to no evidence of ongoing mergers or tidal interactions.
