The galaxy presents as a concentrated, elliptical morphology, appearing largely smooth with a dominant central bulge. The light profile suggests a relatively uniform distribution of older stellar populations, with a notable lack of distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a moderate overall luminosity, appearing more luminous in redder wavelengths. There is a suggestion of very minor tidal disturbances or interactions in its outer regions, but no obvious indications of an ongoing major merger event. Color gradients within the galaxy are subtle, with the central bulge appearing slightly redder than the outer halo. The galaxy presents with a fairly round shape.
