The galaxy appears as a generally smooth, elliptical-like structure, with a concentrated central bulge. The color profile suggests a dominance of older stellar populations, indicated by the yellowish-red hue. There are no obvious spiral arms or dust lanes visible at this resolution, further supporting a classification towards the elliptical end of the Hubble sequence. The galaxy exhibits a degree of elongation, appearing somewhat "in-between" round and cigar-shaped. There is no visual evidence of ongoing major mergers or significant tidal disturbances, suggesting that it is relatively isolated or has already undergone a process of dynamical relaxation. The outer regions fade gradually, indicating a lack of sharp edges or defined boundaries. Overall, the galaxy presents a picture of a mature, relatively quiescent system, possibly an early-type galaxy with a moderate amount of star formation occurring within.
