The galaxy presents as a centrally concentrated, oblate spheroid, displaying a smooth morphology. The light distribution suggests a relatively old stellar population. The major axis extends noticeably further than the minor axis, implying a significant ellipticity. There is a color gradient observable, with the central bulge exhibiting a yellowish-orange hue, possibly indicative of older, redder stars and dust presence. The outer regions, while fainter, show a slight bluer tinge, suggesting some recent star formation. There is no apparent spiral arm structure or significant dust lane features discernible in this image. The overall appearance indicates a galaxy somewhere along the spectrum of lenticular to elliptical type. The shape is not perfectly elliptical, showing slight deviation from the central bulge as it gets more and more circular, indicating possible minor disturbance.
