The galaxy presents as a slightly elongated, disk-shaped structure with a noticeable bulge. The color gradient suggests a complex stellar population distribution. A brighter, yellower central region likely corresponds to an older stellar population, with a faint disk extending outwards. There is some evidence of diffuse blue emission tracing potential star formation regions within the disk. The galaxy appears inclined relative to our line of sight, the lack of clear spiral arm structure could indicate a lenticular morphology or a galaxy undergoing a period of quiescence in its star formation. The overall shape suggests a relatively evolved system. The degree of asymmetry present might imply a past or ongoing minor merger event.
