The galaxy presents a generally smooth, elliptical morphology. It appears largely spheroidal in shape, with a high degree of central concentration. There is a lack of apparent spiral arm structure or prominent dust lanes. The central region exhibits a yellowish hue, suggesting an older stellar population or the presence of dust. Moving outwards, the color becomes slightly bluer, though the change is subtle, and the galaxy generally shows a redder color than blue. There is little indication of active star formation on a large scale. Subtle irregularities or minor disturbances cannot be entirely ruled out, but the overall impression is of a galaxy that has largely settled into a stable configuration, with any recent merging activity likely only very minor. The object appears quite compact, with a concentrated light profile.
