The galaxy presents as a generally smooth, elliptical morphology. It exhibits a high degree of elongation, appearing cigar-shaped, with the major axis significantly exceeding the minor axis. The color profile suggests a dominant population of older stars, with a redder hue particularly concentrated in the central bulge. There's a subtle gradient in color and surface brightness, indicating a higher density and potentially a more active stellar population toward the core region, while the outer regions display a gradual fading and redder color. There is no obvious evidence of spiral arms, dust lanes, or significant star-forming regions within this field of view.
