The galaxy presents as a roughly elliptical, luminous object with a smooth, diffuse morphology. Its color profile suggests the presence of both older stellar populations, contributing to the redder hues, and pockets of relatively recent star formation, which manifest as bluer, greener tones. The central region is noticeably brighter, indicative of a concentration of stars and potentially an active galactic nucleus. There are no discernible spiral arms or distinct morphological features beyond the overall smooth distribution of light. The galaxy does not seem to be significantly interacting or merging with any other galaxies.