The galaxy presents an overall elongated, cigar-shaped morphology. A central, concentrated bulge region exhibits a yellowish-orange hue, indicative of an older stellar population. This bulge is surrounded by a fainter, somewhat diffuse disk. Faint, bluish regions are visible within the disk, potentially indicating areas of recent star formation. No distinct spiral arm structure is readily apparent. There is no visual evidence of ongoing major mergers or significant tidal disturbances, though some slight asymmetry exists within the disk. The galaxy appears relatively smooth in its light distribution, with a higher concentration of older stars.
