The galaxy presents as a somewhat elliptical structure, exhibiting a generally smooth appearance. The central region appears significantly brighter than the outer edges, suggesting a concentration of older stellar populations. The galaxy displays a discernible blue tinge, particularly in the surrounding areas, which indicates the presence of younger, hotter stars and potentially ongoing star formation. While largely smooth, there is a subtle irregularity in the overall form, hinting at a possible past interaction or minor disturbance. The galaxy appears moderately massive, with evidence of active star formation at a modest rate.
