The galaxy presents an overall smooth morphology with a dominant cigar-like shape. The light is concentrated towards the center, which appears a yellowish-white, indicating a significant population of older stars. Moving outwards, the galaxy's color shifts subtly towards a green-blue hue, suggesting the presence of a younger, hotter stellar population in these outer regions. The lack of clearly defined spiral arms or a prominent disk structure supports the classification of this galaxy as primarily smooth. There appears to be no major merger or strong tidal disturbance, though a minor asymmetry hints at potential past interactions. The galaxy is moderately elongated and has no signs of being a point source.
