The galaxy presents a generally smooth, rounded morphology. The central region is noticeably brighter and appears nearly spherical in shape, exhibiting a concentrated luminosity. The outer regions diffuse outwards from the bright central region, suggesting a decrease in stellar density or an increased presence of dust. There appears to be no distinct spiral arm structure or prominent dust lanes visible, consistent with a relatively featureless disk or spheroidal galaxy. It seems to exhibit colors that suggest a population of older stars, but also some bluer colors in the center that might indicate a small region of more recent star formation. There's no visual evidence of any major ongoing merger activity or significant tidal disturbances.
