The galaxy appears to be a relatively small, edge-on spiral, exhibiting a distinct elongated shape. The visible light suggests a composition that is largely older, redder stars, though there are regions of bluer light indicating pockets of recent star formation. A central bulge is present but not particularly prominent, with fainter spiral arms extending outwards. It's disk is not smooth, rather there are obvious disturbances that suggest it may be undergoing minor gravitational interactions with other objects or experiencing internal dynamics causing the observed features. No clear central bar structure is discernible. Overall, the galaxy seems to be relatively undisturbed with a fairly low current star formation rate.
