The galaxy presents as a generally smooth, elliptical-like structure. Its central region exhibits a high degree of luminosity, appearing as a bright, concentrated core. Moving outwards from the center, the luminosity gradually decreases, forming a diffuse halo that lacks distinct, well-defined spiral arms or other prominent features. The overall color profile suggests a population dominated by older stars, with subtle reddish hues distributed throughout, particularly within the central bulge. The elongation of the galaxy indicates a somewhat cigar-shaped morphology, rather than a perfectly spherical distribution of stars. There is no clear evidence of ongoing major mergers or significant tidal disturbances in its immediate vicinity based on the current image resolution. The outer edges of the galaxy appear to fade smoothly into the background, suggesting a relatively quiescent stellar population in the outer regions.
