The galaxy presents as a roughly lenticular structure viewed nearly edge-on. There's a noticeable central bulge that appears yellowish, possibly indicating an older stellar population within. A flattened disk extends outwards from the bulge. This disk appears bluish, suggesting the presence of younger, hotter stars and possibly active star formation regions. The galaxy exhibits some irregularities, showing some features or disturbances, possibly suggesting minor gravitational interaction or recent accretion events. There may be a small tidal tail visible as well. Overall, it appears to be a mid-mass galaxy with ongoing, but not exceedingly vigorous, star formation.
