The galaxy appears to be an elliptical galaxy with a smooth, concentrated light profile. The galaxy exhibits an elongated, cigar-shaped morphology, indicating a possible deviation from perfect sphericity. The core of the galaxy displays a bright, yellowish hue, suggesting an older stellar population. The outer regions of the galaxy appear fainter and exhibit a slightly redder color, which could indicate the presence of dust or older, cooler stars. There is no clear evidence of spiral arms or significant star formation regions.
