This galaxy exhibits a generally smooth morphology, with a structure that appears elliptical. The galaxy presents an overall cigar shape, suggesting a significant ellipticity. The light profile smoothly declines from a brighter, more concentrated central region, indicating a relatively old stellar population concentrated towards the core. There may be some very subtle distortions, but these are minor and the galaxy does not appear to be undergoing any major interactions or mergers. Overall, the galaxy appears to be a relatively undisturbed system, without prominent disk features or spiral arms.
