This galaxy exhibits characteristics of an elliptical morphology, with a smooth light profile and a notable absence of spiral arm structures. The object's shape is somewhat elongated, deviating from a perfectly circular form. Light distribution appears concentrated toward the center, suggesting a dense galactic nucleus. Evidence of a possible minor interaction or disturbance is present, indicated by a secondary, less prominent concentration of luminosity adjacent to the main galactic body. The main component of the galaxy displays a yellowish-white hue, possibly indicative of an older stellar population. The secondary object shows a redder hue, potentially hinting at ongoing star formation, though its exact nature warrants further investigation.
