The galaxy presents as a moderately bright, elliptical morphology with a smooth appearance. The central region exhibits a concentrated luminosity, gradually diminishing outwards into the galaxy's halo. The light distribution suggests a relatively homogenous stellar population. The overall color is slightly reddish, indicative of a population of older stars. There is no readily apparent presence of spiral arms, dust lanes, or distinct star-forming regions. The galaxy appears relatively isolated, with no clear signs of tidal interactions or ongoing merger activity. Its shape is elongated, indicating that it is viewed at an angle.