The galaxy presents a somewhat elliptical morphology, appearing primarily smooth with a high degree of central concentration. The light distribution indicates an evolved stellar population, with a dominant redder hue throughout the galaxy body. However, subtle bluer tones suggest pockets of ongoing star formation, though these are not particularly prominent. There is evidence of disturbance to the main form, implying perhaps past or current gravitational interactions or minor mergers. Further analysis of higher-resolution imagery would aid in confirming the presence of faint tidal tails or other interaction signatures.
