The galaxy exhibits a predominantly smooth morphology, with a high degree of roundness. The central region shows a concentrated luminosity, appearing nearly spherical. There is indication of a possible minor disturbance or merging event in progress, characterized by asymmetry in the galaxy's halo or potential tidal features. The galaxy displays a color gradient, with a tendency towards redder hues in the outer regions. Overall, it is a fairly bright galaxy, suggesting a substantial stellar population.
