The galaxy presents as an elongated, cigar-shaped structure with a smooth, diffuse appearance. The central region exhibits a higher surface brightness than the outer edges, suggesting a concentration of stellar mass toward the nucleus. The color gradient appears relatively uniform across the galaxy, with a slightly bluer hue in the central region, indicating a higher concentration of young stars. The overall morphology suggests an elliptical galaxy with a minimal presence of spiral arms or dust lanes. There is no indication of major disturbances or tidal features indicative of recent mergers, although minor asymmetry in the outer regions cannot be ruled out. Based on its shape and color, the galaxy appears to be an early-type system with a relatively low rate of star formation.
