The galaxy presents as a somewhat elongated, cigar-shaped structure. It appears relatively smooth, with minimal apparent spiral arm structure or distinct features indicative of active star formation. The color gradient suggests a potentially older stellar population, although a faint blueish hue may indicate some ongoing star formation. There is no obvious evidence of a major merger event. The galaxy shows indications of some minor disturbances. The galaxy's core is only slightly brighter than the surrounding galactic halo.
