The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology with a high degree of central concentration. Its overall shape is elongated, resembling a cigar shape, and suggesting an E4-E6 classification on the Hubble sequence. There is no prominent spiral arm structure visible. The central bulge is bright and blends smoothly into the outer regions. There may be a faint disk. The galaxy exhibits a color gradient, with the central regions appearing yellower and redder, indicating an older stellar population, and the outer regions appearing bluer, suggesting the presence of some younger, hotter stars. There's no obvious signs of a recent major merger or tidal disruption. Evidence suggests some minor disturbance is possible.
