The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears predominantly elliptical, with a noticeable lack of distinct spiral arm structures. The light distribution suggests a fairly even decrease in brightness from the core outwards, which would be expected for an elliptical. The object's color is generally consistent, showing a yellowish hue overall, indicative of an older stellar population, with minimal evidence of significant ongoing star formation. There are slight irregularities in the outer regions of the galaxy suggesting some tidal interactions with another galaxy. The galaxy's apparent lack of a prominent disk structure further supports its classification as an elliptical galaxy.
