This galaxy appears to be an intermediate system, exhibiting characteristics of both elliptical and spiral galaxies. The primary component is a large, relatively smooth bulge with a yellowish-orange hue, indicative of an older stellar population. This bulge exhibits an approximate circular symmetry, though it is slightly elongated in one direction. 

A secondary, bluer component is located nearby, potentially interacting with the main body. This region is significantly bluer, suggesting the presence of younger, hotter stars. This secondary structure is more compact and defined, appearing as a distinct and brighter feature. There is some faint asymmetry noted in the overall shape. This asymmetry and the presence of the distinct blue component suggests a possible ongoing minor interaction, where the distinct blue component may be an active star forming region. Evidence for any well-defined spiral arms is absent. 
