This galaxy presents as a relatively compact object, displaying a somewhat elongated, disk-like morphology when viewed from our perspective. A prominent central bulge region is observed, appearing denser and brighter than the surrounding galactic disk. This bulge exhibits a reddish hue, suggesting an older stellar population.

The surrounding disk is composed of bluer material, indicative of ongoing or recent star formation. There may be hints of faint spiral arm structures within the disk, although these features are not distinctly pronounced. The galaxy appears to be largely isolated with no obvious signs of tidal interactions or major mergers, though slight asymmetry may hint at minor past interactions. Overall, the galaxy shows characteristics consistent with an intermediate stage of galaxy evolution.
