The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its core presents a bright, yellowish hue, suggesting a population of older stars and potentially a supermassive black hole actively accreting material. There's little evidence of spiral arm structure or significant dust lanes. The galaxy's overall shape is generally round, with only a slight deviation toward an elongated form. There are no obvious signs of ongoing major mergers or significant tidal disturbances impacting its structure. Faint extensions of diffuse light may suggest the presence of a tenuous halo surrounding the main body.
