The galaxy presents as a somewhat elliptical, lenticular-like structure. The central region is characterized by a concentrated, bright nucleus exhibiting a largely smooth morphology. Proceeding outward from the nucleus, there is a gradual fading of luminosity indicating a relatively homogenous stellar population distribution, with the exception of some slight minor disturbances that are not indicative of any major merging events. There appears to be no prominent spiral arm structure or intense star-forming regions within the visible spectrum. The galaxy's color indices suggest a slightly older stellar population, with a redder color indicating the presence of evolved stars.
