The galaxy appears as a relatively smooth, centrally concentrated object. The light profile suggests a lack of prominent spiral arms or a well-defined disk structure. It exhibits a slightly elongated shape, deviating marginally from a perfectly circular morphology. There is a color gradient, the core of the galaxy appears more yellow, which suggests an older stellar population. There is a diffuse halo surrounding the galaxy, indicating a gradual decrease in stellar density with increasing distance from the galactic center. The overall appearance suggests a galaxy that may be of the elliptical type, potentially a lenticular or an early-type spiral with a bulge that dominates the light. There are no signs of significant ongoing star formation, active galactic nuclei activity, or interaction with other galaxies. The outskirts do not show evidence of tidal streams or disrupted morphology.
