The galaxy appears as a centrally concentrated, generally smooth object. Its color is predominantly yellowish-white, suggesting an older stellar population. The overall morphology appears elliptical, with a high degree of radial symmetry. A subtle color gradient is observed, with the central region exhibiting a slightly more intense yellow hue compared to the outer regions, potentially indicating a higher concentration of older stars towards the center. There is a possibility of a very faint, diffuse halo extending beyond the main body of the galaxy, but this is difficult to ascertain definitively given the image resolution. No distinct spiral arm structures or prominent dust lanes are visible. There may be very minor disturbances. There is an absence of bright, blue star-forming regions suggesting a low ongoing star formation rate. The galaxy presents as a largely quiescent system.
