The galaxy presents as a slightly elongated, disk-like structure. A central bulge is readily apparent, exhibiting a yellowish-white color, suggesting a population of older, cooler stars. The disk itself appears relatively smooth, lacking prominent spiral arm structures. There is evidence of a faint, bluish halo surrounding the central region. The outer regions of the disk show a more subtle gradient of color, transitioning towards bluer hues, indicative of younger, hotter stars and ongoing star formation within the disk. Overall, this galaxy presents a moderately inclined disk orientation with a dominant central bulge and a relatively smooth, featureless disk, suggesting a later-type spiral or potentially a lenticular classification. There is only minor evidence of any tidal disturbances or interactions.
