The galaxy presents as an elongated, cigar-shaped structure. Its overall color profile leans towards warmer hues, with a concentration of yellowish-orange light in the central bulge region. Fainter, bluer emissions extend along the major axis, possibly indicating regions of more active star formation within a disk-like component. There are no prominent spiral arms or distinct morphological features readily apparent. The galaxy displays a moderate degree of smoothness in its light distribution, suggesting a relatively evolved stellar population and/or a face-on orientation that obscures finer details. The luminosity is moderate, given the limited resolution, and the color index suggests an intermediate redshift. There is no obvious visual evidence of a major ongoing merger, though some minor tidal disturbances cannot be ruled out.
