The galaxy presents as a primarily smooth object, exhibiting a centrally concentrated luminosity profile. The overall shape appears elongated, leaning towards a cigar-like morphology. There is no obvious spiral arm structure or defined disk. Some subtle asymmetry or minor disturbances are present, suggesting the potential for past interactions or mergers, however, it does not display clear evidence of ongoing major merger activity. The light distribution suggests a dominant bulge component, with what may be a fainter, extended halo. The galaxy's color indices reveal bluer light in the central region, indicative of possible ongoing star formation, although at a relatively low rate.
