The galaxy presents as a moderately compact object with an overall rounded morphology. The light distribution appears relatively smooth, with a subtle suggestion of a central concentration. While no distinct spiral arm structures are discernible, there may be a slight asymmetry or faint feature hinting at a disk component. Evidence of any major mergers or tidal disturbances appears to be minimal, although there is a very slight distortion visible. The galaxy exhibits an apparent color gradient, transitioning from a slightly bluer hue in the central region to a redder periphery. 
