The galaxy presents a generally smooth and rounded morphology. It appears to be an elliptical galaxy, potentially of type E3-E5 due to its apparent ellipticity. The light distribution suggests a concentrated core, with the luminosity decreasing gradually towards the outer regions. The galaxy exhibits a yellowish hue, potentially indicating an older stellar population with a lower rate of star formation. There is no apparent dust lane or spiral arm structure discernible within the resolution limits of the image. Based on the general morphology, the galaxy seems to be relatively undisturbed, without any major signs of ongoing or recent merger activity.
