The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light profile transitions smoothly from a bright, unresolved core outwards. The overall shape is approximately elliptical, with a slight elongation that could indicate a minor axis. There is a subtle color gradient apparent, with the central region appearing slightly bluer compared to the outer regions which trend towards redder hues. No distinct spiral arms, bars, or prominent dust lanes are discernible. There are no signs of recent major merger activity or tidal distortions, but there is evidence of minor disturbances in the outskirts of the galaxy.
