The galaxy presents as a slightly tilted disk galaxy with an apparent ellipticity. The galaxy exhibits a concentrated bulge, emitting a yellowish light, suggesting an older stellar population in that central region. Surrounding the bulge is a disk, showing a bluer hue, potentially indicating regions of ongoing star formation. There appears to be some level of disturbance or asymmetry within the disk. Faint spiral arm structures may be present, although not clearly defined. The galaxy lacks prominent dust lanes. Its overall morphology suggests a galaxy undergoing some form of interaction or potentially an evolved spiral transitioning towards a lenticular structure.
