The galaxy presents as a slightly elongated, centrally concentrated object. The primary color is a dominant yellowish-orange, suggesting an older stellar population with relatively little ongoing star formation. The galaxy appears smooth in texture, lacking prominent spiral arms or distinct features indicative of active star formation regions such as HII regions. There is a subtle color gradient, with the core appearing more yellow and the outer regions fading into a dimmer, slightly bluer hue. This gradient suggests a radial variation in stellar age or metallicity, with older, more metal-rich stars concentrated toward the center. There is no obvious evidence of a recent merger event or significant tidal disruption, although subtle disturbances cannot be entirely ruled out at this resolution.
