The galaxy presents as a relatively smooth, elliptical-like structure. It appears mostly featureless with no distinct spiral arms or a prominent disk. The central region exhibits a high concentration of light, suggesting the presence of a significant galactic bulge or an active galactic nucleus. The galaxy is somewhat rounded in shape but appears to have some slight elongation. There is no obvious evidence of ongoing major merging activity, although some minor asymmetry or disturbance might be present, especially near the bottom of the galaxy. The color profile suggests a general lack of significant recent star formation across the galaxy, with the galaxy likely containing a population of older stars and perhaps a lower rate of current star formation overall.
