The galaxy presents an overall smooth, elliptical morphology with an apparent cigar-like shape. A bright, concentrated nucleus dominates the central region, exhibiting a yellow-white hue, suggesting a population of older stars. Fainter, slightly bluer emission extends from the central region, potentially indicating the presence of some ongoing, though not intense, star formation activity. There is a region nearby that may indicate an ongoing minor disturbance or possible satellite galaxy interaction. The galaxy appears relatively isolated, showing no strong signs of major ongoing merger activity. The overall color gradient implies a relatively mature stellar population, although hints of bluer regions suggest some pockets of younger stars.
