The galaxy presents as a relatively compact object with a smooth, elliptical morphology. Its core exhibits a concentrated luminosity gradient, suggesting a high stellar density. The overall color profile leans toward the redder end of the spectrum, implying an older stellar population with reduced ongoing star formation. Evident are potential signs of an ongoing or past merger event with another galaxy. The center of the galaxy is noticeably bright and the galaxy as a whole appears to be quite large. The central region presents a concentrated luminosity gradient, which is a characteristic of ellipticals. There are not any spiral arms.
