The galaxy presents as a somewhat amorphous, disk-like structure with a noticeable central bulge. It is elongated and appears to be tilted relative to our line of sight. A diffuse, faint halo surrounds the central region. The color gradient suggests a younger stellar population in the outer regions of the disk, trending towards redder hues in the central bulge, indicative of older stars. There is a hint of clumpy structure, possibly suggesting ongoing star formation regions or spiral arm segments that are unresolved at this resolution. The overall morphology leans towards a late-type spiral or possibly an irregular galaxy. HI data is present for this galaxy, indicating ongoing activity. There appears to be evidence of minor galactic interactions or disturbances as one side of the galaxy has a slightly altered shape.
