The galaxy presents as a somewhat elliptical structure with a prominent, bright central bulge. The galaxy exhibits a smooth overall appearance, with a high degree of central concentration. The color profile indicates a redder core region transitioning to slightly bluer outer regions, suggesting a mix of stellar populations. There is no clear evidence of spiral arms or a well-defined disk. There is a subtle asymmetry in the light distribution. A faint hint of disturbed morphology can be perceived, possibly hinting at a past or ongoing interaction. There also appears to be some faint tidal tail-like light extending outwards on the right.
