The galaxy appears as an elongated, cigar-shaped structure with a central, bright core exhibiting a yellowish-orange hue. The light distribution suggests a relatively smooth morphology with some indication of internal structure. The major axis of the galaxy is significantly longer than the minor axis, indicating a possible edge-on or highly inclined disk-like system. The central bulge seems to be a dominant feature, contributing significantly to the overall luminosity. Faint, diffuse extensions are possibly present beyond the main body, particularly on the left, though their nature is uncertain. The color gradient across the galaxy body suggests potential variations in stellar populations or dust obscuration. The light emanating from this galaxy is consistent with an older stellar population.
