The galaxy appears as a single, relatively compact object with a bright central region. The overall form is somewhat irregular, with evidence of a disk-like structure. The color distribution indicates some variation in stellar populations across the galaxy, the core of the galaxy appears more yellow, potentially indicating older stars. The disk regions show hints of bluer hues, suggestive of more recent star formation. There may be interaction with another galaxy, or an internal disturbance. The overall morphology suggests possible signs of a past merger or ongoing interaction.
