The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable elongation. Its light profile appears centrally concentrated, with a gradual decline in brightness towards the outer regions. The galaxy exhibits a yellow-white hue, suggesting a stellar population dominated by older, redder stars, which is consistent with an elliptical morphology. There is little evidence of prominent spiral arms or significant dust lanes. The smooth appearance indicates it is likely an older galaxy, with a diminished rate of ongoing star formation. It displays a slight asymmetry, possibly hinting at a past minor merger event, though the galaxy appears largely undisturbed. Overall, the galaxy appears as a typical elliptical or lenticular galaxy at a moderate redshift.
