The galaxy presents as a relatively smooth, elliptical-like structure, generally round in appearance. A concentrated central bulge dominates the light profile, exhibiting a bright, yellowish hue that suggests an older stellar population. There is little evidence of spiral arms or significant dust lanes. The outer regions of the galaxy fade gradually into the background sky, indicating a lack of sharp edges or distinct features. The overall color gradient suggests a redder, more evolved population of stars toward the center, with a subtle shift towards bluer colors in the outer regions. This indicates the potential presence of some younger stars, although star formation activity appears subdued. There is no obvious indication of a major merger event, but a minor disturbance cannot be entirely ruled out based on this image alone.
