The observed galaxy presents a somewhat elliptical morphology. Its light profile appears smooth and centrally concentrated, exhibiting a gradual decrease in surface brightness with increasing radial distance from the nucleus. The color appears to shift from yellow to white towards the center of the galaxy, possibly indicating a concentration of older stellar populations in the bulge region. No distinct spiral arm structures or prominent dust lanes are discernible in this image. There is evidence of possible minor disturbances to the shape.