The galaxy presents a relatively smooth, elliptical morphology. Its core exhibits a concentrated, yellowish-white luminosity, suggestive of an older stellar population. The galaxy gradually diffuses outward, maintaining an elliptical shape, with a decreasing surface brightness. Faint bluish hues are observed in the outer regions, possibly indicating regions of younger, hotter stars or ongoing star formation, though at a relatively low rate. The galaxy appears to lack prominent spiral arm structures or significant dust lanes. Its overall appearance suggests a transition type object, between a spiral and an elliptical galaxy. The galaxy appears fairly isolated with no signs of interactions or mergers.
