The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. There's a notable lack of prominent spiral arms. The central region exhibits a bright, concentrated luminosity, suggesting a potentially active galactic nucleus or a dense stellar population. The galaxy displays a slight color gradient, transitioning from a bluer hue in the central regions to a subtly redder shade in the outer areas, indicating potential variations in stellar populations or dust content across the galaxy's structure. The outer edges appear somewhat diffuse and indistinct, hinting at a gradual fading of stellar density. There appears to be some level of tidal disturbance, with the shape being slightly irregular.