The galaxy appears as a somewhat compact object. It possesses a bright, concentrated central region, potentially indicative of an active galactic nucleus or a dense stellar population in the bulge. The surrounding region displays a fainter, diffuse glow which fades out smoothly with no visible spiral arm structures or a clear disk component. There are subtle color variations across the galaxy, with bluer tones concentrated in the central part, suggesting younger stellar populations or ongoing star formation. The galaxy exhibits subtle signs of distortion or irregularities in its shape, possibly resulting from gravitational interactions. There may be a faint, extended halo surrounding the galaxy, further suggesting past interaction events. The overall morphology appears to resemble an elliptical or S0 type galaxy, but with a slight degree of disturbance.
