The galaxy appears as a lenticular or early-type spiral galaxy. It is elongated, presenting a cigar-like shape, and is relatively smooth in texture, without prominent spiral arms or distinct features. The galaxy exhibits a subtle central bulge that gradually fades into the outer regions. The color profile suggests a mature stellar population with little active star formation, indicated by a higher proportion of redder hues throughout the galaxy. There may be only minor disturbances visible in the galaxy's structure, and no evidence of an ongoing major merger.
