The galaxy presents a generally smooth appearance, with a lack of prominent spiral arms or intricate dust lane structures. It exhibits a slightly elongated, cigar-like morphology rather than a perfectly circular form. A bright, concentrated central bulge dominates the galaxy's core, gradually fading into a more diffuse outer region. The color profile suggests a population of older stars, evidenced by the redder hues concentrated towards the bulge. There is minimal evidence of active star formation regions within the observable wavelengths. The overall structure implies a relatively quiescent galaxy that has likely undergone significant evolutionary processes, perhaps a transition from a spiral to a more elliptical form. There may be some minor gravitational interaction or tidal disruption.
