The galaxy presents as a relatively smooth, elliptical structure. Its overall form appears elongated, with the major axis significantly exceeding the minor axis. The central region exhibits a concentrated, bright core, which transitions into a fainter, diffuse halo. The color profile suggests a population of older stars, as evidenced by the reddish-yellow hue dominant throughout the galaxy. Faint blue tinges can be seen in the outer edges of the galaxy. No distinct spiral arms or dust lanes are readily apparent. There is no obvious sign of major interactions or mergers. The galaxy's morphology is largely undisturbed, implying a settled state.
