The galaxy presents as a relatively smooth, elliptical-like structure. There's a centrally concentrated brightness gradient, suggesting a higher density of stars and matter toward the galactic core. The overall color appears to be on the redder side, which could indicate an older stellar population with fewer young, blue stars, or a higher redshift. There are no distinct spiral arms or dust lanes visible, leading to the hypothesis that this could be an early-type galaxy, potentially an elliptical or lenticular. The galaxy exhibits a slight elongation or asphericity, deviating from a perfectly circular shape. There are no obvious signs of ongoing major mergers or significant tidal disturbances. Faint, subtle extensions or a halo might be present, surrounding the main body, but this is difficult to ascertain definitively given the image resolution.
