The galaxy presents as a lenticular or early-type spiral, possibly an S0 type. It is elongated in shape, exhibiting a relatively smooth and homogenous light distribution. The lack of prominent spiral arms and the subtle, diffuse nature of its disk indicates a potentially older stellar population, with lower levels of ongoing star formation. The galaxy is oriented at an angle, presenting an elongated, cigar-like appearance. No signs of major merger events or strong tidal distortions are readily apparent. There is a possible slight disturbance in the symmetry, which could imply minor interactions with neighboring galaxies in the past. The overall color suggests a redder population of stars indicative of an older stellar population, which is often linked with higher mass galaxies that have ceased star formation long ago.
