The galaxy presents as a relatively smooth, elliptical object. Its light profile exhibits a concentrated central bulge with a gradual decrease in intensity towards the outer edges. The central region displays a yellowish-red hue, likely indicative of an older stellar population. Moving outward from the center, a subtle blueish tinge appears. This may suggest pockets of younger stars.

The overall shape appears elongated, with an approximate axis ratio that deviates substantially from unity. There is no clear evidence of spiral arm structure or a well-defined disk component in this image. The absence of significant dust lanes further reinforces its classification as a galaxy lacking substantial ongoing star formation, consistent with its estimated redshift. There is no clear evidence of any ongoing major mergers, however there is a slight irregularity in the overall shape. 