The galaxy appears to be an elongated, disk-shaped system viewed at a significant inclination. It exhibits a relatively smooth morphology, with little evidence of distinct spiral arms or prominent star-forming regions within the observed bands. The overall color suggests a stellar population that is not dominated by young, hot stars, implying a relatively low specific star formation rate. The galaxy's elongated shape appears to be a cigar-shaped, with no major mergers or disturbances. There seems to be some slight dust lanes or other subtle features that contribute to a slightly irregular texture across the disk. The central region exhibits a slight concentration of light, suggesting a possible bulge component. The system presents a coherent structure without significant signs of tidal interactions or ongoing major merger activity.
