The galaxy appears as a smooth, elongated structure. Its shape is roughly elliptical, with a noticeable cigar-like, asymmetric form. The central region shows a slight concentration of light, suggesting a possible core or bulge. The color profile indicates a generally older stellar population, predominantly with light in the redder wavelengths. There is a hint of bluer light in the surrounding regions, indicating some younger stars or ongoing star formation. There are possibly minor disturbances or asymmetries in the outer regions, implying previous minor interactions. There is no obvious disk-like structure visible, and it shows no signs of major merging activity, although there is a slight possibility of a minor disturbance in the outer regions. Overall, the galaxy presents itself as a relatively quiescent system.
