The galaxy appears to be an elliptical galaxy, displaying a smooth, diffuse morphology. It exhibits a radial gradient in luminosity, being brightest at its center and gradually fading outwards. The galaxy presents an elongated shape, with the major axis significantly longer than the minor axis, resembling a cigar shape. There is little evidence of spiral arms or prominent dust lanes, suggesting a lack of significant recent star formation. The galaxy's color is primarily yellow-orange, indicative of an older stellar population. No signs of ongoing merger activity or tidal disturbances are readily apparent. The galaxy appears relatively isolated, without close companions that would suggest strong gravitational interaction.
