The galaxy presents as a moderately bright object with a discernible elliptical morphology. The central region exhibits a concentrated and luminous core, displaying a yellowish hue, suggestive of an older stellar population. A fainter, bluer region is visible adjacent to the main body, possibly indicative of ongoing star formation within a disturbed or tidal structure. The galaxy lacks clear spiral arm structures. There is potentially a minor merger or interaction happening with the bluer object. The overall appearance suggests a relatively smooth light distribution, although some irregularities are present.
