The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse morphology. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The galaxy's shape is somewhat elongated, approaching a cigar shape, but is more closer to an intermediate shape. There is little evidence of spiral arms or prominent dust lanes. The color suggests an older stellar population, with a yellowish hue dominating the galaxy's light, which is consistent with minimal ongoing star formation. There are no indications of recent or ongoing major merger events or significant tidal disturbances.
