The galaxy presents as a slightly elliptical, relatively smooth structure with a concentrated central bulge. The core exhibits a yellowish-white hue, indicative of an older stellar population. A subtle, less concentrated disc surrounds the bulge, displaying a more complex color profile with hints of green and traces of red. These colors suggest the presence of ongoing, albeit moderate, star formation within the disc region. The galaxy appears relatively isolated and unperturbed, displaying no obvious signs of tidal interactions or recent mergers, although a subtle asymmetry in the outer edges may suggest a past interaction or minor disturbance. Overall, the galaxy appears as a transitional object between a spiral and elliptical type, with characteristics of both, hinting at a dynamically evolved system.
