The galaxy presents a generally smooth morphology, suggestive of an elliptical type or a spiral galaxy viewed at a high inclination angle. Its overall shape appears moderately elliptical, exhibiting a deviation from a perfectly circular form. There is a concentration of luminosity toward the center, forming a bright nucleus region that gradually diffuses outwards. The color distribution across the galaxy's body appears relatively uniform with a slight color gradient. There is very little evidence of distinct spiral arm structures, prominent dust lanes, or other features typically associated with actively star-forming galaxies. The outer edges of the galaxy fade gradually into the background, without any sharp cut-offs or distinct boundaries. The galaxy's structure appears largely undisturbed, without any obvious signs of ongoing mergers or significant tidal interactions. Minor disturbances cannot be ruled out based on the image data alone.
