The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution with no discernible spiral arm structure. The core is noticeably bright and concentrated, suggesting a higher density of stars in the central region. The galaxy appears elongated, with a cigar-shaped form and a dominant axis. The color profile indicates a redder hue, potentially indicative of an older stellar population with fewer young, blue stars and ongoing star formation. There is no obvious evidence of any major ongoing merger activity, nor a significant tidal disturbance in its structure, suggesting a relatively quiescent state in its evolutionary history.
