The galaxy exhibits a complex morphology, presenting features characteristic of both elliptical and spiral galaxy types.

A prominent central bulge dominates the galaxy's core, appearing smooth and relatively featureless with a yellowish hue, suggesting an older stellar population. This bulge appears to be elongated.

There is evidence of a faint, extended disk. This disk is oriented roughly edge-on. The disk component appears slightly bluer, particularly at the edges, which may indicate the presence of younger, hotter stars and ongoing star formation within these regions.
 
A possible merger or tidal interaction seems plausible, given the disturbed morphology.
