The galaxy presents as a somewhat elliptical, smooth object with a concentrated central bulge. There appears to be very little, if any, evidence of spiral arm structure or prominent dust lanes. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region. There may be a slightly bluer component in the outer regions, however this is difficult to discern. The overall morphology indicates a high probability that the galaxy is an early-type, potentially an elliptical galaxy. There is no clear indication of ongoing major mergers or significant tidal disturbances. The shape deviates somewhat from a perfect circle, leaning toward an elliptical form, though not exceedingly elongated.
