The object appears to be a spiral galaxy, with a prominent central bulge. While not exceptionally bright, the core appears somewhat active. Two distinct spiral arms emanate from the central bulge, one being the major arm, the other being a short spur. The spiral arms are loosely wound, with a grainy appearance, indicating ongoing star formation. The central bulge has an elongated shape, potentially indicating the presence of a bar structure, though not particularly strong or prominent. There is no evidence of significant morphological disturbance or major merging events. The galaxy is face-on, which helps make it look like it is a spiral galaxy. Overall, the galaxy exhibits characteristics of a relatively normal, though not exceptionally massive, spiral galaxy undergoing moderate star formation.
