The galaxy appears to be a relatively smooth, disk-like structure, with a central bulge that is somewhat bright and compact. The galaxy has a slightly elongated morphology, exhibiting a shape that is somewhere between round and cigar-shaped. There is little evidence of strong spiral arm structure. The color gradient suggests a dominant older stellar population. While appearing relatively undisturbed, there is a hint of possible minor interaction, based on some slight asymmetry within the disk. Overall, the object is a mature galaxy with evidence of past or ongoing star formation.
