The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits an elliptical morphology, with the isophotes appearing generally regular, but with a very slight deviation from perfect circularity. The color profile appears to be redder in the central regions, transitioning to slightly bluer hues in the outer parts. There is no obvious presence of strong spiral arm structure or prominent dust lanes. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances with nearby companions, nor are there indications of recent starburst activity based on the lack of intense blue emission or irregular morphology. The overall impression is that of a galaxy composed primarily of older stellar populations, with a likely suppressed star formation rate.
