The galaxy presents as a relatively compact object with a smooth, centrally concentrated light profile. Its shape appears to be roughly elliptical, with a suggestion of slight elongation, but the image resolution limits a more precise morphological classification. The color is generally consistent across the galaxy, with a subtly redder hue, indicating a potentially older stellar population. There appears to be no obvious evidence of strong spiral arm structures, bright star-forming regions, or a prominent dust lane, suggesting that this galaxy is a relatively quiescent system. There are some indications of a minor gravitational disturbance on the periphery.
