The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution is generally consistent with an elliptical classification, showing a gradual decrease in intensity outwards from the core. There is no clear evidence of spiral arms or a distinct disk component. The galaxy's color appears moderately blue in the center fading outwards, suggesting possible ongoing star formation, or a population of relatively young stars, though the smooth appearance does not suggest current star formation. The overall shape is close to round. There's no visible sign of significant tidal disturbance or interaction with another galaxy, and the outer regions show a gradual fading rather than sharp truncation, indicating it is not currently undergoing a major merger.
