The galaxy presents as a relatively compact object, exhibiting a moderate degree of ellipticity. It displays a generally smooth morphology with minimal evidence of spiral arm structures or distinct features. The central region appears concentrated, suggesting a possible bulge component. The color profile indicates a presence of older stellar populations, with a possible indication of recent star formation. There is a hint of a possible gravitational interaction or minor merger event, as evidenced by a possible disruption of the galaxy's symmetric shape. Overall, the galaxy appears to be undergoing an interaction, with a generally smooth profile that also presents signs of recent star formation.
