The galaxy presents as a slightly elongated, cigar-shaped form. It appears to be relatively smooth in structure, lacking prominent spiral arms or distinct features. The light is concentrated toward the center of the galaxy, suggesting the presence of a central bulge. The color gradient shifts from a central yellowish hue, possibly indicating an older stellar population, to a bluer tint towards the outer edges. This suggests the presence of more recent star formation in the galactic disk. There is no strong evidence of significant ongoing merging activity or major disturbances. The galaxy exhibits a moderate redshift, indicating a considerable distance.
