The observed galaxy exhibits an overall elliptical morphology, although a definitive classification remains challenging due to the presence of internal structures. The galaxy presents a bright, concentrated central bulge, exhibiting a luminosity gradient that diminishes towards the outer regions. A faint, diffuse halo surrounds the central bulge, showing a mottled texture, indicative of possible tidal streams or dust lanes.

There appears to be some distortion in the outer disk, suggesting a possible gravitational interaction. Furthermore, regions of enhanced blue color within the disk are observed. These likely correspond to areas of ongoing star formation. The spiral arm structure is ill-defined but shows hints of fragmented arms. These arms do not appear to be highly structured, giving the galaxy a somewhat flocculent appearance. The object appears to be possibly interacting, as evident from the tidal features.
