The galaxy presents as a relatively smooth, elongated structure. A central bulge exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluish regions extend from the central bulge, possibly indicative of ongoing star formation within a disk-like component. There may be evidence of a faint disk, viewed edge-on or at a steep inclination. Overall, the galaxy appears to be relatively undisturbed, showing no signs of major mergers or tidal interactions, but there may be very slight asymmetry in the outer regions.
