The galaxy presents as a somewhat elliptical, moderately smooth structure. The color distribution appears uneven, with a central concentration of redder hues that become slightly more blue as it extends further away from the central bulge. This may indicate a mix of stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars in the outer regions, and the hint of some star formation. There's a suggestion of minor tidal disturbance in the outer regions, though this is tentative. The overall shape does not appear highly distorted, and there is no clear evidence of ongoing major merger activity. It is a reasonably luminous galaxy and possesses a sizable mass. It is likely in the process of slowing down star formation.
