The galaxy presents a generally smooth morphology, with a concentrated central region of high luminosity. The overall shape appears approximately round, though there is a subtle elongation. The color profile is redder in the central regions, indicating an older stellar population and/or significant dust obscuration. Fainter, diffuse extensions can be observed, with bluer tints, possibly denoting regions of ongoing, low-level star formation activity. There are hints of disturbances in the structure of the galaxy, which could be indicative of past interactions.
