The galaxy appears to be elliptical or lenticular in morphology, exhibiting a largely smooth light distribution without prominent spiral arms or a well-defined disk structure. The overall shape is generally rounded, presenting a mild ellipticity. The central region exhibits a concentration of luminosity, appearing brighter and more condensed than the outer regions. There is evidence of possible tidal disturbance. There also appears to be a nearby object, though the relationship between the two objects is unclear. The galaxy exhibits a color gradient, with the central regions appearing redder, possibly indicative of an older stellar population, and the outer regions show a bluer hue, which could signify the presence of younger, hotter stars.
