The galaxy presents an elongated, cigar-shaped morphology. Its central region exhibits a concentrated, brighter luminosity, appearing smooth and relatively featureless. Progressing outward from the core, the luminosity gradually decreases. Subtle color variations are visible, with a slight shift towards bluer hues observed in the outer regions compared to the more yellow/red central bulge. There's no obvious spiral structure or strong evidence of current major merger activity, although subtle irregularities might suggest minor tidal disturbances or interactions. The galaxy's overall smooth appearance and color profile suggest a moderate level of star formation.
