The galaxy presents as a relatively small, elongated structure. A prominent, centrally located bulge region appears smooth and exhibits a pale blue hue. This color suggests the presence of a younger stellar population within the bulge, potentially indicating recent or ongoing star formation, although this could also be affected by redshift. Extending outwards from the bulge, there appears to be some disk-like structure, although it is faint. The disk component displays a more yellow-red color compared to the bulge. This color shift may indicate an older stellar population in this region. It is unclear what type of galaxy this is based on the image, but there is likely a minor merger happening with a smaller galaxy below it.