The galaxy presents as an elongated, cigar-shaped structure with a somewhat smooth overall appearance. A brighter central bulge region is discernible, gradually fading into the surrounding galactic disk. The disk exhibits a subtle blue hue. The galaxy lacks any obvious spiral arm structures or significant dust lanes, suggesting it is primarily composed of older stellar populations with a low star formation rate. There is no evidence of any major tidal disturbances or ongoing mergers, indicating a relatively isolated and undisturbed system.
