The galaxy presents as a highly elongated, cigar-shaped structure. Its light distribution appears relatively smooth, indicating a lack of significant star-forming regions or distinct spiral arms. The color profile suggests a redder hue overall, consistent with an older stellar population and potentially lower levels of ongoing star formation. There are no prominent dust lanes or other morphological features indicative of recent mergers or significant disturbances. The galaxy's overall appearance is indicative of a lenticular or elliptical galaxy viewed edge-on.
