The galaxy appears to be a relatively small, elongated spiral galaxy, likely seen nearly edge-on from our vantage point. Its central bulge is not particularly prominent, suggesting a smaller black hole or a less dense concentration of stars at its core. The disk of the galaxy displays subtle signs of structure, with hints of spiral arms visible, indicating a relatively active star formation rate within the disk. There might be a minor gravitational interaction occurring. The galaxy's overall color suggests a mix of stellar populations, with both older, redder stars and younger, bluer stars contributing to its overall light. 
