This galaxy presents as a somewhat elongated, cigar-shaped structure. Its light appears relatively smooth with no obvious spiral arm structure or strong knots of star formation visible in the image. The central region appears brighter and more concentrated. There are hints of a subtle color gradient, with the core showing bluer hues possibly indicating recent star formation and the outer regions appearing redder, suggesting an older stellar population. Overall, the galaxy appears relatively undisturbed, though there may be a very minor interaction that cannot be determined through imaging alone. The galaxy is a medium sized galaxy, likely with a relatively low rate of star formation.
