The object presents as a relatively small, luminous galaxy, exhibiting a primarily smooth morphology with a high degree of central concentration. The galaxy appears predominantly round, with a subtle elongation. Light distribution across the galaxy is quite uniform. Evident asymmetry suggests possible gravitational interactions or disturbances, with indications of potential tidal features or a past merger event. A possible indication of a weak tidal stream or an unusual feature can be seen on its top right. The color composite indicates a moderate age stellar population, showing a higher presence of older, redder stars. It is possible this galaxy is in the late stages of merging with another galaxy, or has completed a minor merger event and is disturbed as a result.
