The galaxy presents an overall smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a slightly elongated shape, not perfectly spherical, with an intermediate roundness. There appears to be no significant merging activity or major disturbances evident in its structure. The galaxy displays a color gradient, transitioning from a bluer central region to slightly redder hues in the outer regions. This could indicate a population of younger, hotter stars in the core and older, cooler stars in the outskirts. The apparent size is relatively small, suggesting it is a distant galaxy. The integrated light suggests a moderate stellar mass. The moderate star formation activity in the galaxy suggests the blue colors of the central region may be evidence of ongoing star formation.
