The galaxy presents a morphology indicative of an elliptical type. Its overall shape is moderately elongated, appearing somewhat rounded with a slight cigar shape. The light distribution is relatively smooth, with no prominent spiral arms or distinct features suggesting active star formation regions. There is very little visible dust obscuration. The galaxy's color profile indicates an older stellar population, as inferred from the redder hue, suggesting minimal recent star formation activity. Possible minor disturbances hint at a past or ongoing interaction with another galaxy, although a major merger seems unlikely based on the overall smoothness of its structure.
