The galaxy presents as a moderately luminous object, exhibiting characteristics of both smooth and somewhat disrupted morphology. The dominant light distribution appears centrally concentrated and has a pronounced red-yellow hue with a slight extension, suggesting an elliptical shape that is not perfectly spherical. There is a slightly brighter and bluer knot to the upper right from the galaxy's center, possibly indicative of a region of more intense star formation. Overall the disk is ill defined and not particularly spiral in nature. There also appears to be a slight disturbance to the shape, which may indicate a past or ongoing minor interaction, or a recent merger, even though it is not strongly disturbed. The galaxy's color suggests the presence of an older stellar population, with a relatively low rate of ongoing star formation.
