The galaxy presents as a centrally concentrated object with a smooth overall morphology. The light distribution suggests a roughly elliptical shape, although some irregularity is present. A central, brighter region is clearly visible, surrounded by a more diffuse and less luminous halo. The color gradient moves from a pinkish core to a blue-green outer region, which suggests possible variations in stellar populations.

The smooth morphology dominates, with little evidence of distinct spiral arms or a bar structure. Some faint, disturbed light surrounding the main body suggests a potential minor interaction or tidal features, although this is not definitive. It seems that this galaxy has had or is experiencing little to no merging activity.

The galaxy's half-light radius is estimated to be several kiloparsecs. Based on light emission, the galaxy appears to be undergoing star formation at a moderate rate. Based on colour, star formation seems to be taking place in areas in the outer region of this galaxy.
