The galaxy presents an overall elongated, cigar-like morphology. The light distribution is smooth and centrally concentrated, suggesting a lack of prominent spiral arms or other significant substructure. The color gradient shifts from a bluer hue at the outer regions to a more red/yellow color towards the center of the galaxy. This could potentially indicate a younger stellar population in the outer regions and an older population concentrated towards the core. There are subtle signs of minor disturbances in the galaxy's morphology, with possible faint distortions in its overall shape. However, there is no strong evidence of a major merger event or tidal interactions. The galaxy appears relatively isolated, without any obvious nearby companions.
