The galaxy presents as a moderately bright object with a concentrated central bulge. It appears elliptical in shape, though the limited resolution does not permit a detailed analysis of its morphology. The galaxy exhibits a relatively smooth appearance, with little indication of strong spiral arms or significant dust lanes. A slight elongation is observed, hinting at a possible disk component or triaxial shape, but this requires further investigation. The galaxy's color is somewhat redder in the DESI bands, potentially indicating an older stellar population and/or significant dust reddening. There is a noticeable lack of intense star formation regions within the galaxy itself, consistent with a lower specific star formation rate. There is no indication of a major merger event. Minor disturbances cannot be ruled out but are not visible.
