The galaxy presents as a disk-shaped system, elongated in appearance, suggesting an oblate spheroidal or lenticular morphology viewed at a high inclination. The central region exhibits a brighter, reddish hue, possibly indicative of an older stellar population or dust obscuration. Extending outwards from the core, a bluer, more diffuse component is observed, potentially representing areas of ongoing star formation within the galaxy's disk. The overall light distribution appears relatively smooth, with no prominent spiral arm structures or distinct features easily discernible. The galaxy does not seem to be undergoing major merger events, but minor disturbances cannot be ruled out. The galaxy's morphology is cigar shaped.
