The galaxy exhibits a predominantly smooth morphology, appearing largely elliptical in shape, although there is evidence of some disk-like features or irregularities within its structure. Its overall form is somewhat elongated, approaching a cigar shape. There is a possible merging event occurring with another object on its side. The galaxy presents a color gradient, shifting from a bluer hue in its outer regions to a warmer, more yellowish central bulge. This suggests a potential difference in stellar populations, with younger, bluer stars populating the outer regions and older, redder stars concentrated in the center. The presence of some disturbed or irregular structure could be indicative of interactions or past merger events affecting the galaxy's shape and stellar distribution. Overall, it is a relatively compact galaxy with a moderate level of activity or disturbance.
