The galaxy presents a generally smooth morphology, appearing largely featureless in the image. It exhibits a centrally concentrated luminosity profile, suggesting a prominent bulge component. The overall shape is moderately elliptical, deviating slightly from a perfect circular form. The color profile indicates a redder hue, particularly towards the central region, potentially indicative of an older stellar population and/or significant dust extinction. There is a subtle suggestion of a faint disk component, but it's not clearly defined. No prominent spiral arms or bar structures are discernible. The absence of strong blue colors implies a relatively low ongoing star formation rate. There might be minor tidal disturbances present.
