The galaxy presents as a generally smooth object with a slightly elongated, cigar-like morphology. The central region exhibits a high concentration of light, appearing bright and yellowish, suggesting an older stellar population. Extending outward from the core, the galaxy exhibits a more diffuse and fainter halo or disk-like structure. There are subtle hints of blueish light present in the outer regions, indicating the presence of some younger, hotter stars. The overall structure shows no prominent spiral arms or significant disturbances, suggesting a relatively quiescent system. There is no evidence of a major ongoing merger or tidal interaction.
