The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, centrally concentrated light distribution. The light profile transitions smoothly from a bright, yellowish core to a fainter, more diffuse outer region with a slightly redder tint. Its shape is elongated, appearing somewhat cigar-shaped. There is little evidence of spiral arms or a distinct disk structure. A minor, greenish-blue asymmetry is observed on one side, which could potentially indicate tidal disturbance or interaction with another galaxy, however there is not obvious evidence of a major disturbance, like a tail. The overall color suggests a relatively older stellar population with low levels of ongoing star formation. 
