The galaxy presents a generally smooth and concentrated morphology. It appears elliptical in shape, with a moderately elongated profile. The central region exhibits a high surface brightness, suggesting a dense concentration of stars. The galaxy's color profile indicates a mix of stellar populations, with a dominant population of older, redder stars contributing to the overall yellowish hue. There appears to be some evidence of bluer star forming regions, perhaps an indication of ongoing star formation. However, these regions are not prominent, suggesting a relatively low star formation rate. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy does not appear to be undergoing a major merger event or significant tidal disruption.
