The galaxy presents as a roughly elliptical object, exhibiting a centrally concentrated luminosity profile. A bright, unresolved core dominates the galaxy's appearance. The light from the core has a relatively blue hue, indicating a population of hot, young stars, or potentially non-stellar emission. The central region is surrounded by a slightly less luminous area, also with a predominantly blue color. This implies ongoing or recent star formation within this inner region. Moving outwards, the galaxy appears to have a faint, diffuse halo. This outer structure transitions to redder colors, suggesting an older stellar population with fewer newly formed stars compared to the central region. There is a subtle suggestion of asymmetry or a possible minor perturbation in the overall morphology, indicating a potential past interaction or merger.
