The galaxy presents as a slightly elliptical, centrally concentrated object. The core region exhibits a yellowish hue, suggestive of an older stellar population. The outer regions transition to a bluer tint, possibly indicating ongoing star formation. There is a lack of distinct spiral arm structures or a well-defined disk. Some faint irregularities are present, but there does not appear to be any major ongoing merger events. The overall appearance favors a relatively smooth morphology.
