This galaxy presents as a somewhat elongated, cigar-shaped structure. There is evidence of a relatively smooth morphology, with a high fraction of the light appearing to be diffuse and not concentrated in distinct spiral arms or other features. The galaxy exhibits a color gradient, with a slightly bluer hue towards the upper section, transitioning to a warmer, redder color in the lower section. This color variation might indicate differing stellar populations or dust content across the galaxy, with potentially younger, hotter stars dominating the bluer region and older, cooler stars, and perhaps dust obscuration, contributing to the redder region. There might be signs of minor tidal disturbances, although it is likely that no major merger event is happening. The galaxy appears to be relatively isolated.
