The galaxy presents an asymmetrical morphology, appearing to exhibit both smooth and disk-like features. A dominant, somewhat elongated central bulge is visible, displaying a yellowish-orange hue suggesting an older stellar population. Extending from this central region, there are hints of a fainter, bluer disk. The overall light distribution is not uniform. There appears to be some degree of internal structure or dust lanes partially obscuring the central bulge. Faint distortions are observed in the outer regions of the galaxy, possibly indicating tidal interactions or recent mergers. There is a possible secondary bright region of the galaxy, indicating some form of galactic interaction.
