The galaxy presents an overall smooth, elliptical morphology, with a major axis noticeably longer than its minor axis, suggesting a classification towards the elliptical end of the Hubble sequence. It exhibits a moderate redshift, indicating a considerable distance. The light distribution is centrally concentrated, becoming fainter towards the outer regions. The observed color is predominantly yellowish-orange, potentially indicating a stellar population dominated by older, redder stars, which is consistent with a lower rate of star formation. There is no strong evidence of spiral arm structure or prominent dust lanes visible in the image. The galaxy's shape is elongated, showing a cigar-like form. There's no visual sign of any ongoing major merger activity or significant tidal disturbances. The galaxy appears relatively undisturbed in its present state.
