This galaxy exhibits a generally elliptical morphology, although with hints of a disk-like structure. The light distribution appears relatively smooth, lacking strong spiral arm features. The galaxy's color profile suggests a population of older stars, giving it a yellowish hue. The axial ratio indicates that it is somewhat elongated and cigar shaped, rather than perfectly round. There is no obvious evidence of a major merger event, although the slight disturbances may indicate minor gravitational interactions. Overall, this galaxy presents characteristics consistent with an intermediate type, possibly an early spiral or lenticular galaxy, exhibiting characteristics somewhere between a typical elliptical and spiral morphology.
