The galaxy presents as a largely smooth, elliptical structure with a concentration of light towards the center, indicative of a prominent galactic bulge. The color profile suggests a population dominated by older stars, likely exhibiting a redder hue compared to galaxies with active star formation regions. There appears to be minimal evidence of spiral arms or significant dust lanes. The overall appearance is consistent with an early-type galaxy that has largely ceased active star formation. It appears to be a singular system, with no obvious signs of a major merger or significant tidal disturbances. There is a very faint patch of light to the left of the main galaxy, but it's unclear whether this is connected or a separate background object.
