This galaxy presents as a spiral galaxy, viewed at an oblique angle to our line of sight. The central bulge is prominent and moderately sized, appearing bright and concentrated, suggesting a substantial population of older stars. 

Spiral arms are visible, although somewhat disrupted and diffuse. They extend outwards from the central bulge. Hints of a bar structure might exist, but it does not appear to be particularly strong or well-defined.

There's evidence of ongoing star formation within the disk, particularly along the spiral arms, indicated by bluer regions. However, the overall star formation rate appears to be relatively moderate.

The galaxy exhibits signs of a possible minor interaction or disturbance, with some asymmetry in the spiral arm structure. However, there are no clear indicators of a major merger event or significant tidal disruption. The colors suggest a mix of stellar populations, with a contribution from both older, redder stars in the bulge and younger, bluer stars in the disk.
