The galaxy presents as a compact object with a moderately bright central region, possibly indicative of a concentrated stellar population or active galactic nucleus. The overall morphology appears somewhat amorphous and disturbed. There is faint, extended emission surrounding the central body, with some asymmetry noted in its distribution. The galaxy has a blue hue which indicates the presence of young, hot stars. While there is no clear spiral structure, there is an absence of a truly elliptical shape. The surrounding extended emission exhibits faint, irregular wisps and patches, potentially signifying tidal features or ongoing interactions with nearby systems, though the primary object dominates the image. Given the irregularities, there may be recent or ongoing star formation events contributing to the observed color profile.
