The galaxy presents as a single, largely homogenous object with a generally elliptical morphology. The central region exhibits a bright, concentrated core that transitions smoothly outward into a less luminous halo. The color profile suggests an older stellar population, as the dominant hues are in the redder portion of the spectrum. There is little evidence of distinct spiral arms or active star-forming regions, with the overall texture appearing smooth. The galaxy may exhibit some minor tidal disturbances based on asymmetries in the outer halo region, but is generally undisturbed. The bulk of the galaxy appears relatively relaxed and quiescent.
