The galaxy appears as a relatively smooth and centrally concentrated object. It exhibits a generally elliptical morphology, with the light distribution gradually decreasing from the core outwards. There is a subtle elongation, but it is mostly round in appearance. No prominent spiral arms, bars, or dust lanes are readily discernible. The galaxy's color suggests a relatively evolved stellar population. There is no strong indication of recent or ongoing major star formation. The galaxy does not show any signs of major disturbances, such as tidal tails or significant asymmetries, suggesting it is not currently undergoing a major merger. There is a faint, irregular structure nearby, suggesting the possibility of a minor interaction.
