The galaxy presents an elongated, cigar-shaped morphology. It exhibits a noticeable central bulge that appears relatively bright and concentrated. From the color gradients, the galaxy has a redder hue at the core, suggestive of an older stellar population dominating the central region. Moving outwards from the core, there's a transition to slightly bluer hues, particularly at the edges, which might indicate the presence of younger stars in these outer regions. There is little indication of prominent spiral arm structures or well-defined dust lanes.
