The observed galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. Its shape is elongated, presenting an oblate spheroid with a noticeable ellipticity. The light profile indicates a high Sersic index, suggesting a steeper decline in surface brightness compared to exponential disk galaxies. The color gradient transitions from a bright, yellowish central bulge to fainter, redder outer regions. There may be faint tidal features indicative of past interactions. The galaxy exhibits a low star formation rate. No significant dust lanes or spiral arm structures are discernible in the image.
