The galaxy presents as a lenticular or possibly a highly inclined spiral galaxy, exhibiting a smooth, elongated morphology. Its color profile is relatively uniform across the visible structure, appearing largely white or slightly yellowish, which may indicate an older stellar population with reduced ongoing star formation. The galaxy's apparent size is quite small, suggesting a considerable distance. There is no obvious evidence of spiral arm structure or significant dust lanes. The absence of prominent blue regions suggests a lack of significant recent or current star-forming regions. Slight asymmetries or minor disturbances within the galaxy's light distribution might hint at past or ongoing gravitational interactions, but this remains uncertain based on this image alone. The high concentration of light suggests this galaxy is most likely an elliptical galaxy.
