This galaxy exhibits a generally elliptical morphology, appearing smooth and relatively featureless. It presents a concentrated central bulge that is bright and yellowish in color, suggesting an older stellar population. The galaxy's overall color profile shifts towards redder hues from the center outwards, which may indicate a gradient in stellar age or metallicity. There is a slight elongation, with an axis ratio appearing close to 3:1. This could indicate that it's likely an elliptical galaxy type, however, it might be a highly inclined spiral galaxy, given its flattened shape. There is no obvious evidence of spiral arms or a disk structure discernible within the data presented, nor does it indicate ongoing or recent major merger activity. A slight asymmetry might be visible, however, its difficult to say definitively whether this is a real feature, or simply a visual artifact. Given the smooth appearance and color, this galaxy may have a relatively low star formation rate.
