The galaxy presents a largely smooth, elliptical morphology. Its color is predominantly yellowish-orange, possibly indicative of an older stellar population with reduced ongoing star formation. The galaxy exhibits a centrally concentrated luminosity profile, with the brightness decreasing gradually toward the outer regions. There are no visible spiral arm structures or prominent dust lanes that would suggest a disk component. A faint, slightly elongated structure is visible nearby, potentially a companion galaxy or a background object. The overall appearance suggests a massive system. The absence of blue light implies a relatively low specific star formation rate.
