The galaxy presents an overall elongated, cigar-shaped morphology, indicating it is likely an elliptical galaxy viewed edge-on or a highly inclined spiral galaxy. It exhibits a smooth, diffuse light distribution, with a bright central bulge and fainter, extended outer regions. There is no visible structure such as spiral arms or dust lanes. The color appears to be a relatively uniform bluish-white, suggesting a population of generally older, evolved stars with a low on-going star formation rate. There is no obvious evidence of tidal interactions or major disturbances in its structure. The galaxy appears relatively isolated, with no close neighboring galaxies visible. The estimated size is approximately 5.6 kpc, placing it within the range of typical dwarf galaxies.
