The galaxy presents as a somewhat diffuse, elliptical structure, though with hints of a disk. The central bulge is bright and appears relatively smooth, exhibiting a yellowish-orange hue, suggesting an older stellar population. Moving outward from the bulge, the galaxy's color transitions to a more bluish tint, possibly indicating the presence of younger, hotter stars in the outer regions. There are slight indications of spiral arms or disk features, but they appear somewhat disrupted or ill-defined. The overall morphology suggests a possible recent or ongoing interaction, or internal disturbances within the galaxy. The outer edges of the galaxy are less defined, gradually fading into the background sky, indicating a less dense stellar population in these regions.
