This galaxy exhibits a morphology suggestive of a disk galaxy viewed at a slight inclination. A faint, diffuse disk is observable, with a central bulge that appears relatively bright.  The disk demonstrates some structural features and is not entirely smooth, indicating the presence of internal processes such as star formation regions. The general shape suggests a substantial fraction of the galaxy's light is emitted from a structured disk component, rather than a purely spheroidal system. There may be minor gravitational disturbances, indicating a possible interaction with a smaller companion.  While no distinct spiral arm structure is readily apparent in this image, the slight irregularities within the disk could indicate their presence or remnants thereof. The galaxy appears generally bluish in hue, which might indicate ongoing star formation.
