The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density, potentially including an active galactic nucleus. The colour profile is generally red-yellow, indicative of an older stellar population, with potentially suppressed star formation. There are no immediately obvious spiral arms or significant dust lanes visible. The galaxy appears relatively undisturbed with no major merging activity detectable in this image. Overall, the galaxy is an elliptical type system dominated by an older stellar population.
