The galaxy appears to be a relatively smooth, elongated structure. Its morphology is suggestive of an elliptical or lenticular galaxy, exhibiting a generally featureless profile. The central region displays a concentrated luminosity, potentially indicating a dense galactic nucleus. The color gradient transitions from a brighter, yellowish core to a redder, less intense outer halo, which may indicate the presence of an older stellar population, with some dust, or a degree of redshift. There is no apparent evidence of distinct spiral arms or a prominent disk structure. It shows a relatively undisturbed morphology, which indicates there may be low levels of recent star formation, if any. The overall shape is elongated, deviating significantly from a perfectly circular morphology.