This galaxy exhibits a generally smooth morphology, with a pronounced central bulge. The object appears elongated, presenting a cigar-shaped profile. There is no evident disk structure, but there are minor disturbances surrounding it. The galaxy presents a yellowish-white hue, potentially indicative of an older stellar population, possibly in the early stages of transitioning into a redder phase. No substantial dust lanes or prominent star-forming regions are discernible. The galaxy seems to exist as a relatively isolated entity, without any visually obvious indications of ongoing or recent major merger events.
