The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, centrally concentrated morphology. The light distribution suggests a fairly homogenous stellar population. There is a clear color gradient, with a yellowish-white core transitioning to bluer hues in the outer regions. The galaxy appears moderately elongated, displaying a cigar-like shape rather than a perfectly circular form. There are no distinct spiral arms or other features indicative of active star formation in the disk, but subtle color variation suggests some ongoing or recent star formation in the outer regions. There is no evidence of a major merger or significant tidal disturbances affecting the galaxy's structure.
