The galaxy presents as a relatively faint, elongated structure. Its morphology appears disk-like, though not particularly well-defined, and is more likely a spiral or lenticular. There's some evidence for spiral arms, which look like they're tightly wound. The center of the galaxy has a bright, concentrated bulge. The galaxy shows a hint of bluer, star-forming regions, possibly indicating ongoing star formation. However, the overall redder color suggests an older stellar population and/or significant dust obscuration. There might be some subtle signs of tidal disturbances or interactions, such as a very faint asymmetry in the outer regions.