The galaxy presents as a moderately inclined, disk-like structure. The central region exhibits a concentrated, bright, yellowish core, suggestive of an older stellar population or significant dust obscuration. Surrounding this core, a fainter, bluer disk is visible. The blue color implies the presence of younger, hotter stars and ongoing star formation within the disk. The disk appears somewhat disturbed or irregular, possibly indicating a minor gravitational interaction or recent merger event. There is no obvious spiral arm structure, indicating that this could be a lenticular galaxy. Overall, the galaxy demonstrates a mix of old and young stellar populations, with hints of recent or ongoing activity.
