The galaxy presents as a relatively smooth, elliptical morphology. The object exhibits a centrally concentrated luminosity profile with a gradual decrease in brightness extending outwards. There is an absence of distinct spiral arms or prominent dust lanes, suggesting an older stellar population and a lack of significant ongoing star formation. The galaxy appears nearly circular in shape, showing minimal ellipticity. There are no signs of tidal disturbances or ongoing mergers with other galaxies. The color index suggests a redder overall spectral energy distribution. The size of the galaxy is somewhat compact. Overall, the galaxy appears as a mature, quiescent system with properties consistent with an elliptical classification.
