The galaxy presents as a centrally concentrated, largely featureless object with a generally smooth morphology. The central region exhibits a yellowish hue, suggesting an older stellar population. This color gradually transitions to a bluer, though still subdued, periphery. There is a notable absence of distinct spiral arms or prominent dust lanes. The overall shape is approximately elliptical, showing a slight elongation. Minor disturbances or interactions with other galaxies are not obviously apparent within the observed field, as the overall structure appears relatively undisturbed, though a very small disturbance is possible. The general smoothness implies that the galaxy is of a redder variety with mostly older stars, and lower specific star formation rate.