The galaxy presents as a relatively smooth, elongated structure. There is an indication of a central bulge, characterized by a concentrated, yellowish-orange hue, which might suggest a population of older stars. Fainter, bluish-white regions extend from the central bulge along the major axis of the galaxy, potentially indicating areas of more recent star formation. No distinct spiral arms are discernible. The overall morphology suggests a disk-like galaxy viewed at an angle. No significant tidal disturbances or signs of ongoing major mergers are apparent, with little evidence of asymmetry or irregularities in the shape of the disk.
