The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge that transitions gradually into a more diffuse halo. The color profile suggests a dominant population of older stars, with a yellowish hue, consistent with minimal ongoing star formation. There is no apparent spiral arm structure or distinct dust lanes visible. The galaxy appears fairly symmetrical and does not show significant signs of tidal disturbance or interaction with other galaxies. It appears relatively isolated in the image, maintaining a well-defined, singular structure.
