The galaxy presents an overall elliptical morphology, appearing largely smooth and without prominent spiral arm structures or significant dust lanes. The light profile suggests a concentration towards the center, exhibiting a bright, well-defined core region. The color index suggests a relatively evolved stellar population, with a moderate contribution from younger stars as noted by blue-ish hue in the surrounding halo. The galaxy exhibits a mild degree of ellipticity, deviating somewhat from a perfectly circular shape. There is little to no evidence of any ongoing major merger events or significant tidal disturbances that could indicate recent interactions with other galaxies. Based on the image and data, the galaxy's star formation rate is relatively low.