The galaxy presents an elongated, cigar-shaped morphology. The light distribution is dominated by a smooth, centrally concentrated component, likely a bulge or spheroid. The color appears to have a radial gradient, with a yellowish-white hue at the core gradually transitioning to a bluer tint in the outer regions. There is no clear evidence of spiral arm structure or significant dust lanes visible in the image. The overall appearance suggests a galaxy undergoing a relatively low rate of star formation. Although appearing mostly undisturbed, closer inspection reveals subtle irregularities in the outer regions, hinting at a minor interaction.
