The galaxy presents as a relatively compact, disk-like structure. It exhibits a fairly smooth morphology with a high degree of rotational symmetry. The color distribution suggests a bulge with older stellar populations, surrounded by a relatively flat disk with bluer colors, perhaps indicating regions of more recent star formation. No strong spiral arms are discernible. There is no obvious strong disturbance in morphology, such as tidal tails or obvious merger signatures. Its overall shape appears nearly circular, with only a slight hint of elongation or a cigar-shaped structure. No indications of active galactic nuclei, such as jets or strong emission lines are apparent in this image. Overall, this appears to be a relatively isolated galaxy, characterized by a smooth light distribution and a lack of significant morphological disturbances.
