The galaxy presents as a smooth, elongated structure, displaying a relatively featureless morphology. Its shape is cigar-like, indicating a potential elliptical classification or a disk galaxy viewed at a high inclination. The light distribution appears uniform across the main body, lacking prominent spiral arms or distinct star-forming regions. A subtle color gradient is observed, with a bluer hue noted in the central regions, suggesting the presence of a younger stellar population or recent star formation activity, though limited. There is little evidence of significant tidal disturbances or ongoing mergers with other galaxies.
