The galaxy presents as a singular, elliptical-like object with an overall smooth appearance. The central region exhibits a high degree of luminosity, gradually decreasing towards the outer edges. The galaxy's color profile leans towards the redder end of the spectrum, indicating a population of older stars. A slight asymmetry in the light distribution might indicate a minor interaction or past merger event, though it remains largely undisturbed in its morphology. A faint disk feature might be present on the outer edge of the galaxy. Overall, the morphology suggests a relatively evolved system, possibly with a suppressed star formation rate.