The galaxy presents as an elongated, cigar-shaped structure. It appears relatively smooth in texture. The color distribution suggests a gradient, with the central region appearing more reddish-gold, indicating an older stellar population. There are hints of bluer regions along the outer edges, possibly indicating areas of recent or ongoing star formation. No prominent spiral arm structures or a distinct bulge are readily discernible. The galaxy may be experiencing a minor disturbance, possibly a minor merger or tidal interaction, though definite proof of this is not easily provided.