The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge that appears more yellow in color, suggesting an older stellar population in this region. The galaxy gradually fades in intensity toward its outer edges, transitioning to a redder hue. There is little to no visible evidence of distinct spiral arms or significant dust lanes, indicating a lack of ongoing major star formation or a relatively uniform stellar distribution. Overall, the galaxy seems to possess a fairly regular, somewhat elongated shape, lacking any obvious signs of recent merger activity or significant morphological disturbance.
