This galaxy presents a lenticular morphology, exhibiting a flattened disk structure without prominent spiral arms. It is oriented approximately edge-on relative to our line of sight. The central bulge appears bright and concentrated, displaying a yellowish hue indicative of an older stellar population. A faint, extended disk surrounds the bulge, with a bluer color gradient towards the outer regions, which may indicate ongoing, albeit relatively low, star formation within that region. There are no distinct features suggesting a recent major merger event, although subtle irregularities might be present, warranting further investigation for signs of minor disturbances or tidal interactions. Overall, the galaxy appears to be in a relatively quiescent state.
