The galaxy presents a largely smooth morphology, appearing elliptical in shape. It exhibits a generally rounded appearance, with minimal discernible features disrupting its overall symmetry. The galaxy appears to have a concentrated central region. The color profile suggests an older stellar population, with a greater contribution from redder wavelengths. There is no strong evidence of ongoing major mergers or significant tidal disturbances; the galaxy's structure is largely undisturbed. The galaxy does not display distinct spiral arms or a prominent disk structure, further supporting a classification as an elliptical galaxy. Overall, the galaxy appears to be a relatively quiescent system, likely characterized by lower levels of star formation activity.
