The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its morphology is dominated by a centrally concentrated bulge, with a noticeable lack of spiral arms or prominent disk structures. The light distribution is mostly homogenous, with the majority of light seemingly emanating from the core region. The galaxy exhibits a yellowish-red hue, suggesting an older stellar population with minimal ongoing star formation activity. There is little evidence of dust lanes or patchy star formation regions within the visible spectrum. There is no significant morphological disturbance or sign of any major recent merger events. Overall, the galaxy appears to be a well-defined, quiescent system.
