The galaxy presents a generally smooth morphology, appearing largely featureless upon visual inspection. It exhibits a centrally concentrated luminosity profile, with the intensity decreasing gradually from the core outwards. The overall shape is somewhat elliptical, tending towards a more intermediate form. There is no strong indication of spiral arm structure or a prominent disk. The galaxy appears relatively isolated, showing no significant signs of major tidal distortions or ongoing mergers. The color appears largely uniform across the galaxy, with a bias towards redder hues. There is no pronounced evidence of significant dust lanes or prominent star-forming regions within the galaxy. The lack of bluer colors might suggest a dominant population of older stars. Minor disturbances cannot be ruled out but do not dominate the overall structure.
