This galaxy exhibits a generally elongated, cigar-like morphology. The light distribution appears relatively smooth, with a central concentration of yellowish light suggesting an older stellar population in the galactic bulge. Fainter bluish light is visible towards the outer regions. The overall structure suggests a possible disk galaxy viewed at an inclined angle, though no distinct spiral arms are discernible within the resolution of this image. There are no major disturbances or signs of merging activity readily apparent, though a slight asymmetry is noticeable. The overall shape does show signs of being slightly distorted from a classic elliptical. The galaxy is generally isolated with no nearby objects visible.