The galaxy presents a smooth, elongated morphology, appearing cigar-shaped in projection. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. A slight bluish tint is observed at the outer edges, suggesting possible recent star formation activity in these regions, although the overall color is generally consistent with an older stellar population. There is no noticeable spiral arm structure or prominent dust lanes visible in this image. The galaxy exhibits a degree of internal structure but does not appear to be undergoing any major merging events or significant tidal disturbances.
