The galaxy appears as a relatively smooth, centrally concentrated object. Its color is primarily yellowish-orange, suggesting an older stellar population dominates the light output. There is a lack of distinct spiral arm structure or prominent dust lanes, lending it a rather featureless appearance. The overall shape is largely circular, with no obvious elongation or tidal distortions indicative of recent major merger activity. The galaxy's compact nature suggests a possible classification as an elliptical or lenticular type. The faintness of the object indicates that it is relatively distant. There is little evidence of ongoing star formation based on the color, but it may be possible that there is a small amount hidden inside.
