The galaxy exhibits a somewhat irregular morphology, suggestive of a recent or ongoing interaction or merger event. Multiple distinct luminous concentrations are observed, with a brighter, more centrally located condensation and two less well-defined neighboring regions.

The galaxy appears relatively compact, with a moderate ellipticity, and an average radius of around 6 kpc. Its overall color profile suggests a mixed stellar population, potentially including both older, redder stars and younger, bluer stars.

The luminosity profile of the galaxy is concentrated, with a strong peak brightness in the brightest luminous condensation. This suggests a possible central concentration of stars, potentially a bulge or a nuclear region. Evidence suggests a potential tidal tail or bridge of stellar material extends outward from the main body of the galaxy.
