The galaxy presents an elongated, somewhat cigar-shaped morphology. It is relatively smooth in appearance, exhibiting a lack of distinct spiral arms or other prominent features. A subtle color gradient is observed, with a yellowish hue concentrated at one end of the galaxy and a bluer tint dominating the central and remaining regions. This color variation may indicate differences in stellar populations, with older, redder stars dominating the yellowish region and younger, bluer stars prevalent elsewhere. There appears to be a slightly enhanced brightness in the central region suggestive of a galactic bulge. There is no evidence of any major ongoing mergers or significant disturbances. The faintness of the galaxy indicates that it is not a highly active system.
