The galaxy appears as a centrally concentrated, largely featureless object, exhibiting a generally elliptical morphology. Its light profile appears smooth, without distinct spiral arms or a prominent bar structure. The central region of the galaxy displays a reddish hue, potentially indicative of an older stellar population or dust obscuration. A slight gradient towards greenish-blue is present in the surrounding regions, potentially pointing towards younger star formation or different stellar populations. Overall, the galaxy appears undisturbed, with no significant tidal features or evidence of ongoing major merger activity. It appears as a relatively isolated system. The galaxy appears to be reasonably compact and quite massive.
