The galaxy presents a generally elliptical morphology, although some irregularities are visible. The central region is characterized by a bright, concentrated luminosity profile, suggesting the presence of a significant stellar population. The overall color appears to be relatively red/yellow, possibly indicating a population of older stars, with likely suppressed star formation. There may be a very small hint of spiral structure. The outer regions of the galaxy appear more diffuse. There does not seem to be any major merger events, nor major disturbances in the morphology, although a faint asymmetric structure is noticeable on one edge. The overall appearance suggests a massive galaxy, likely a disk galaxy viewed at an angle, with relatively smooth features and a dominant bulge.
