The galaxy presents as a relatively smooth, elliptical object. Its morphology is predominantly spheroidal, with no discernible spiral arm structure or bar feature. The light distribution appears concentrated towards the center, suggesting a prominent bulge. The galaxy's color profile indicates a redder hue, possibly indicative of an older stellar population with lower ongoing star formation. There is a minor suggestion of disturbance in the galaxy's symmetry, potentially resulting from a minor interaction.
