The galaxy presents a moderately smooth, elongated morphology, appearing roughly cigar-shaped in projection. The light distribution suggests a central concentration with a gradual decrease in intensity towards the edges.  Evidence for a prominent disk structure is not readily apparent, and there are no immediately obvious signs of spiral arms or significant dust lanes.  The galaxy exhibits a relatively blue color, potentially indicative of ongoing star formation. No significant merger activity or tidal disturbances are readily discernible from the morphology. There is a slight increase in brightness in what looks like the central bulge of the galaxy. Overall, the galaxy appears to be an elliptical or lenticular galaxy with some evidence of star formation.
