The observed galaxy presents a notable morphological structure indicative of a potential ongoing or recent interaction. The galaxy displays a generally smooth, elliptical appearance, suggesting a classification towards early-type galaxies, potentially an elliptical or lenticular galaxy. However, there is evidence of asymmetry and possible disturbances in the light distribution. A distinct brighter core is visible, and the isophotes appear somewhat distorted, hinting at a departure from a purely spheroidal morphology. A fainter component is observed, possibly a dwarf galaxy, or tidal debris resulting from an interaction. There is some evidence of minor disturbances within the galaxy. The central region appears more concentrated while the outer regions diffuse outwards. Overall, this galaxy appears to be a smooth galaxy that may be undergoing a merger. 