The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a strong luminosity, indicative of a dense stellar population. Moving outwards from the core, the light intensity gradually decreases.  There is a slight elongation to the galaxy’s shape, deviating minimally from perfect circularity. No distinct spiral arm structure or bar feature is apparent.  The color profile suggests an aging stellar population, as evidenced by a redder hue in the central bulge and a fainter, bluer disk component. The absence of significant dust lanes supports the interpretation of an evolved system undergoing relatively low levels of current star formation. There are no signs of ongoing major merger events or tidal disruptions visible.
