The galaxy presents as a generally smooth, elliptical morphology with a concentrated central bulge. The light profile appears relatively uniform, lacking any distinct spiral arm structures or prominent dust lanes. The color distribution is mostly consistent across the galaxy, tending toward the redder end of the spectrum, indicating an older stellar population and a relatively low star formation rate. The overall structure suggests that the galaxy is likely a mature system. There is no obvious evidence of recent merger activity or significant tidal disturbances. Based on the galaxy's round appearance, it is most likely viewed close to face-on.
