The galaxy presents a lenticular morphology, exhibiting a prominent central bulge that transitions smoothly into a surrounding disk. The bulge displays a yellowish-orange hue, potentially indicative of an older stellar population. The disk appears relatively smooth and lacking in distinct spiral arm structures, with a subtle blueish tint along its edges. The overall shape suggests a moderately elongated, cigar-like form. There is no clear evidence of on-going significant star formation, nor is there evidence of significant merger activity or tidal disturbances. The galaxy appears to be a relatively isolated system.
