The galaxy exhibits a generally smooth morphology, appearing mostly featureless with a slight elongation. It appears to have a central region that is more condensed and brighter than its outer regions. There is some indication of a possible disk, but without clear spiral arm structures, it is difficult to say definitively. The galaxy presents itself as moderately luminous, with light primarily in the green, red, and some blue wavelengths. The shape is intermediate between round and elongated. There is no strong evidence of tidal disturbances or ongoing major mergers. Some subtle asymmetry may be present, hinting at a past or minor interaction.
