The galaxy presents as a smooth, elliptical-like structure, exhibiting a concentrated central bulge that graduates outward into a more diffuse halo. The color profile suggests an older stellar population, dominated by redder wavelengths, possibly indicating a low rate of ongoing star formation. There appears to be little evidence of prominent spiral arms or dust lanes, indicative of a relatively undisturbed morphology. There is no sign of any interactions such as mergers. The overall appearance is consistent with that of a quiescent galaxy, potentially residing within a denser galactic environment.
