The galaxy appears as a roughly elliptical, moderately compact object. It exhibits a bright, concentrated core, suggesting a significant central mass concentration. The outer regions display a fainter, more diffuse halo. The overall color profile indicates a slightly bluer hue in the central regions, possibly indicating the presence of younger stellar populations or ongoing star formation. The outer halo appears redder, hinting at older stellar populations. There is no apparent spiral structure or strong disk component visible, instead showing a generally smooth structure. There may be a very slight distortion in the overall shape, possibly indicating a past or ongoing interaction, but it's not dramatically disturbed.
