The galaxy presents a smooth, elliptical-like morphology with a concentrated central region. The color profile appears to be generally redder, suggesting an older stellar population and reduced star formation activity. There are minor signs of disturbance or irregularities in the outer regions of the galaxy, possibly indicating a past or ongoing interaction. At least one additional object lies in close proximity to the galaxy along the same line of sight, suggesting a potential physical association or merger, though it is not certain.
