The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a generally smooth morphology with no immediately obvious spiral arms or bar features. The light distribution appears centrally concentrated, gradually fading towards the outer edges, with a dominant reddish hue, suggesting an older stellar population with relatively low ongoing star formation. There is a slight suggestion of some faint disk-like component around the center. The galaxy appears largely undisturbed, showing no strong evidence of major mergers or significant tidal interactions, though there is some sign of possible minor disturbance. Its shape is neither perfectly round nor elongated, residing somewhere in between.
