The galaxy presents a generally elliptical morphology, with a high degree of central concentration. The light distribution appears smooth and featureless, indicative of an early-type galaxy, possibly an elliptical or lenticular (S0) type. There is no discernable spiral arm structure or dust lane visible. The central bulge is bright and prominent, with a gradual decrease in luminosity towards the outer regions. The color is generally consistent across the galaxy, trending towards the redder end of the spectrum, suggesting an older stellar population. There is no apparent star forming regions. The overall impression is that of a quiescent galaxy with little to no current star formation activity. There is no evidence of a major ongoing merger. Minor irregularities in the outer halo may indicate past interactions.
