The galaxy presents a largely smooth morphology, appearing elliptical in shape. There is a noticeable concentration of light towards the center, indicating a prominent galactic nucleus or bulge. The color profile suggests an older stellar population, with a yellowish hue dominating the central region. The light appears more blue towards the edge, suggesting that there is possibly a small amount of star formation occurring in the outer edges of the galaxy, though the overall rate of star formation appears low. There's no obvious evidence of spiral arms or significant dust lanes. No major mergers or interactions are clearly visible, though some minor disturbance cannot be ruled out. Overall, the galaxy appears as a relatively undisturbed, evolved system.
