The galaxy presents as a slightly elongated, disk-like structure seen at an oblique angle, possibly approaching edge-on. There's a central bulge region that appears significantly brighter and has a yellowish-orange hue, suggesting an older stellar population or dust obscuration. The disk itself is less luminous and bluer in color, possibly indicating the presence of ongoing star formation. The galaxy exhibits some irregularities in its outer regions, potentially indicative of minor tidal interactions or recent accretion events. There is an unconfirmed object close to the galaxy which could be a part of the galaxy system. The overall appearance suggests a spiral or lenticular galaxy with a complex formation history.
