The galaxy presents as a smooth, centrally concentrated object, appearing elliptical in shape. The light distribution decreases gradually from the core outward, with no discernible spiral arm structures or prominent features such as dust lanes or distinct knots of star formation visible. The color profile is consistent with an older stellar population, displaying a yellowish hue, suggestive of lower levels of current star formation activity and a dominance of evolved stars. There is no evidence of strong tidal distortions or ongoing major mergers, though a possible minor disturbance is not completely excluded. The galaxy's overall morphology indicates it is likely a relatively massive, quiescent system.