The galaxy presents as a relatively compact object, exhibiting a smooth, centrally concentrated morphology. Its overall shape approximates an ellipse, with the ratio of major to minor axis suggesting a moderate degree of ellipticity. The light profile appears smooth with no distinct spiral arm features discernible. The color gradient across the galaxy indicates a yellow/red hue, suggestive of an older stellar population and lower rate of recent star formation. There is some indication of a minor disturbance of the light in the galaxy, though the evidence is not conclusive from this data set. The galaxy does not appear to be actively merging with another galaxy, although it could potentially have had a minor disturbance in its past.
