The galaxy appears as a relatively smooth, elongated structure, suggesting a likely elliptical morphology viewed at a significant angle. The central region exhibits a concentration of light, appearing yellowish in color, potentially indicative of an older stellar population. The outer regions of the galaxy display a bluer hue, albeit less concentrated, which may reflect the presence of a younger stellar population or ongoing star formation activity, though faint. There are no visible spiral arms or distinct dust lanes. The overall structure suggests a system undergoing a moderate level of star formation with an estimated mass range of 10^9.5 solar masses. The object does not appear to be undergoing any major merger activity, with minimal visible signs of tidal disturbances or asymmetries. The cigar-like shape is evident.
