The galaxy presents a concentrated central bulge with a noticeable drop-off in light intensity extending outward, suggesting an elliptical morphology or a spiral galaxy viewed at a high inclination. There appears to be a subtle asymmetry or minor disturbance in its structure, possibly indicating a past or ongoing interaction with another galaxy, though not an obvious ongoing merger. The galaxy's color is predominantly yellow-orange, which is characteristic of older stellar populations. Some regions have hints of bluer light, suggesting pockets of more recent, albeit subdued, star formation. The galaxy exhibits a relatively smooth overall appearance with a lack of prominent spiral arms or dust lanes. The object's shape is more elliptical than circular, leaning towards an intermediate roundness.
