The galaxy exhibits a relatively smooth morphology, presenting a centrally concentrated light profile. It appears somewhat elliptical in shape, with a noticeable asymmetry in its outer regions. The central region is distinctly brighter and bluer than the surrounding areas, suggesting a concentration of younger, hotter stars, or potentially an active galactic nucleus. The light distribution decreases gradually from the center outwards, with a slight elongation evident. There is a faint tail or plume-like feature extending from one side of the galaxy, indicating possible tidal interactions or past merger events. The overall color of the galaxy suggests a mix of stellar populations, with a dominant population of intermediate-age stars contributing to its luminosity.
