The galaxy presents as a lenticular system, elongated in shape, with a high degree of oblateness. The light distribution appears smooth, lacking prominent spiral arm structures. The central bulge is not highly pronounced, blending smoothly into the disk. There is a slight color gradient across the galaxy, with the core region exhibiting a yellowish hue, indicative of an older stellar population. Fainter blue hues are visible at the outer edges of the disk, suggesting a small amount of on-going star formation. No major tidal disturbances or mergers are apparent, with only minor irregularities in the outer regions of the galaxy. The morphology leans strongly towards a highly elongated, cigar-like shape when compared to a perfectly circular form. It seems to be an isolated galaxy, with no obvious signs of interaction.
