The galaxy exhibits a morphology suggesting a relatively smooth distribution of light. The dominant component is a central bulge, appearing spheroidal and characterized by a strong concentration of light intensity. The color of this bulge is primarily yellow, possibly indicating an older stellar population. Adjacent to this bulge, an area of bluer light can be observed, suggesting the potential presence of younger, hotter stars or an active star forming region. The disk, if present, is faint, with no apparent spiral structure. The galaxy appears to be undergoing, or to have recently undergone, a merger event, likely due to the irregular structure of the blue star forming region on the edge of the galaxy. Overall, it is a relatively compact galaxy.
