The galaxy presents a predominantly smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity, indicative of a significant stellar population and potentially a supermassive black hole actively accreting matter.  The light profile appears to diminish gradually from the core outwards, lacking distinct spiral arm structures or prominent dust lanes.  There is a very slight deviation from a perfect sphere, showing it is mildly elliptical in shape. Faint, diffuse extensions of light surround the main body, suggesting a halo of older stars. There is no obvious evidence of ongoing major mergers or strong tidal disturbances, though subtle asymmetries may hint at minor gravitational interactions. The galaxy appears relatively isolated within its local environment. Overall, the galaxy presents a redder hue, signifying a dominant population of older, evolved stars and lower rates of current star formation.
