This galaxy exhibits a pronounced, elongated shape. There appears to be a central bulge, slightly yellowish in hue, which indicates an older stellar population. Extending from the central bulge are fainter, bluish regions, possibly indicative of ongoing star formation within spiral arms or a disk structure. The overall morphology suggests an edge-on spiral or lenticular galaxy, with a relatively smooth appearance, though minor disturbances cannot be ruled out given the slight asymmetry and faint irregularities along its edges. The light distribution implies a system dominated by older stars in the central region, with pockets of younger, bluer stars in the outer regions.
