The galaxy presents a moderately elongated, elliptical morphology. The central bulge exhibits a bright, concentrated luminosity, indicating a high stellar density, likely dominated by an older stellar population as evidenced by the yellowish-orange color. There appears to be a faint disk component. The smooth light distribution and lack of prominent spiral arms or significant dust lanes suggests a relatively quiescent system with low ongoing star formation. The galaxy appears undisturbed, with no clear signs of recent merger activity or tidal interactions.
