This galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth light distribution. Its morphology is neither distinctly spiral nor irregular. The galaxy's color profile indicates a notable concentration of older stellar populations in the central region, characterized by yellower hues. Moving outward from the core, the galactic disk exhibits a slight bluer color indicative of younger stellar populations. The galaxy presents a moderately elongated shape, and there is no evidence of a major ongoing merger, though subtle disturbances cannot be ruled out. There are no clear signs of prominent dust lanes or significant star-forming regions, implying a relatively quiescent state.
