The galaxy appears to be an elliptical type, exhibiting a generally smooth and round morphology. The central bulge region displays a concentrated, yellowish-orange hue, possibly indicative of an older stellar population. There is a slight suggestion of a very faint, diffuse halo surrounding the core. To the left, there is a slightly brighter and bluer object or region, that could indicate the presence of younger stars and/or active star formation there. There is no apparent spiral structure or significant dust lanes visible, suggesting a lack of ongoing major mergers or significant gas content. Overall, the galaxy seems relatively undisturbed and quiescent.
