The galaxy presents a primarily smooth, elliptical morphology. It appears elongated, with a cigar-like shape. The color profile suggests a dominant population of older stars, visible in the reddish-orange hue of the central bulge. There's a slight bluer tinge around the outer edges of the galaxy, potentially indicating some ongoing, albeit low, level of star formation. No clear spiral arm structures or significant dust lanes are visible. There appears to be a small, disturbed area at the top of the galaxy which may represent an ongoing minor merger.