The galaxy presents as a single, dominant object with a centrally concentrated luminosity profile. The overall morphology appears smooth, with a roughly elliptical shape that is neither perfectly round nor significantly elongated. A hint of disk-like morphology is suspected. No prominent spiral arms or bar structures are discernible. The color gradient suggests an older stellar population, appearing reddish to yellow towards the core. No strong evidence of ongoing major merging activity is observed. Marginal evidence of minor disturbance is visible in its morphology. The faint color of the surrounding area suggest the galaxy is not forming many stars.
