This galaxy exhibits a morphology consistent with a disturbed system, potentially undergoing a merger or interaction. The central region displays a relatively smooth luminosity profile. However, there are irregular extensions and asymmetries that suggest gravitational disturbance. These asymmetric features extend outwards from the central body, disrupting any simple spiral or elliptical shape. The galaxy appears to have a central bulge-like component. The overall color profile is complex, showing patches of redder hues intermixed with bluer regions. The bluer regions may indicate areas of more active star formation. The redder components could represent older stellar populations or dust obscuration.
