The galaxy presents as a relatively compact structure with a dominant, bright central bulge exhibiting a smooth, elliptical morphology. There is an extended, fainter disk surrounding the bulge. Within the central region, a very bright concentration of light suggests a possible active galactic nucleus or a region of intense star formation. Colors appear relatively uniform throughout the galaxy, with a slight bluer tint near the edges, possibly indicating the presence of younger stellar populations. There appears to be very minimal disturbances, with no indication of spiral arms or other features associated with on-going merging or tidal interactions. The galaxy appears somewhat lenticular, showing properties intermediate between elliptical and spiral galaxies.
