The galaxy appears as a relatively compact, luminous object. Its morphology is generally smooth, appearing elliptical or lenticular. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy exhibits a mild degree of ellipticity, leaning towards a more rounded shape than a highly elongated form. The color profile suggests a population dominated by older stars, emitting more light in the redder wavelengths of the spectrum. Based on its morphology, it is unlikely that this galaxy is currently undergoing major merger activity, though minor tidal disturbances cannot be completely ruled out. Its relatively small size also suggests a possible dwarf galaxy, or an older, more mature galaxy.
