The galaxy appears to be elliptical in shape, exhibiting a smooth, centrally concentrated light distribution. There is a notable color gradient, with the central region showing a slightly redder hue, suggesting an older stellar population, possibly dominated by red giant stars. Moving outwards, the galaxy gradually transitions to a bluer color profile, hinting at the presence of younger, hotter stars in the outer regions. No distinct spiral arms or prominent dust lanes are visible. Faint irregularities or minor disturbances might exist in the galaxy's outer envelope, but these are not pronounced. The galaxy does not appear to be undergoing a major merger, but the faint irregularities could potentially indicate minor tidal interactions or past accretion events. Overall, the galaxy presents a morphology consistent with an early-type galaxy with moderate star formation activity, predominantly in its outer regions.
