The galaxy presents a generally smooth morphology, appearing as an elliptical or lenticular type. It exhibits a noticeable elongation, with its shape deviating from a perfectly circular form, suggestive of a cigar-like appearance. The central region displays a high concentration of light, indicative of a substantial bulge component. The light distribution gradually fades from the core, indicating a smooth transition toward the outer regions. There is minimal evidence of strong spiral arms or a prominent disk structure. The red-shifted color suggests an older stellar population. There appears to be some form of minor gravitational disturbance or interaction occurring at its edges.
