The galaxy presents as a relatively smooth, elongated structure. It is likely an elliptical galaxy, exhibiting a shape that is significantly more cigar-shaped than round. A faint disk may be present, but the overall morphology suggests a lack of prominent spiral arms. The light distribution appears fairly even across the galaxy, indicating a somewhat homogenous stellar population. The galaxy displays a central concentration of light. Its color is primarily white-ish, suggesting an older population of stars. Some blue regions are also visible, indicating regions of active or recent star formation. There is no visible evidence of any recent or ongoing major merger events.