The galaxy appears as a somewhat elliptical structure with a bright, concentrated central bulge. The color of the bulge is primarily yellow to orange, suggesting an older stellar population. Extending outwards from the bulge is a fainter, less defined disk. There is evidence of bluer regions within this disk, indicating the presence of younger stars and ongoing star formation, although not especially prominent. The galaxy displays a general smoothness in its morphology, with no clear, large-scale spiral arms or significant dust lanes visible. There may be minor disturbances or irregularities in the outer regions of the galaxy, but overall the galaxy seems relatively isolated and undisturbed.
