The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated luminosity, appearing as a bright, yellowish core. Moving outward from the core, the light gradually diffuses into a fainter halo. There is only a faint suggestion of spiral arms or other distinct features within the disk. The overall color profile indicates a relatively evolved stellar population, consistent with a galaxy dominated by older stars. There appears to be very little dust evident in the galaxy. There is no evidence of any major disturbances or ongoing mergers in the system's morphology.
