The galaxy presents as a generally smooth, elliptical-shaped object with a noticeable color gradient. Its core exhibits a bright, concentrated yellowish-white luminosity, suggestive of an older stellar population. Proceeding outward from the core, the light gradually dims to a more reddish hue, potentially indicating a lower concentration of younger, bluer stars in the outer regions. The galaxy appears elongated in a cigar-like shape, lacking any distinct spiral arm structures or defined dust lanes visible at this resolution. Faint irregularities or disturbances are noted on one side, possibly indicative of a minor gravitational interaction or past merger event. Overall the lack of any major ongoing star formation is indicated by the redness of the galaxy. 
