The galaxy presents as a largely featureless, smooth object. Its overall shape appears elliptical or spheroidal, with a high degree of central concentration. The primary color is a yellowish-white, suggesting an older stellar population. Faint blue hues are observed extending from the central region, possibly indicating the presence of some younger, hotter stars, though the rate of star formation appears to be low. There is some suggestion of a very faint, diffuse halo extending beyond the main body of the galaxy. There does not appear to be any evidence of spiral arms, bar structures, or ongoing major mergers. Subtle disturbances, like a faint tidal tail or warping of the disk, could potentially be present but are not clearly resolved in this image. The galaxy seems to be relatively isolated, showing no immediate signs of strong gravitational interaction with other nearby galaxies.
