The galaxy presents as a smooth, elongated structure, appearing cigar-shaped. Its color profile suggests an older stellar population, with a dominant yellow-orange hue in the central regions. The absence of clearly defined spiral arms or significant dust lanes indicates a lack of active star formation. The overall smooth morphology is indicative of a galaxy that has largely exhausted its gas supply. There may be evidence of a very minor disturbance, but the galaxy appears mostly undisturbed. The light distribution is centrally concentrated, dimming gradually toward the edges. The galaxy is likely a massive elliptical galaxy.