The galaxy presents an overall elongated, cigar-shaped morphology. Its light profile appears relatively smooth and centrally concentrated, with a gradual falloff in surface brightness from the core outwards. There is no apparent disk structure or spiral arms, suggesting a primarily spheroidal stellar population. The color index indicates a redder hue characteristic of older stars. There are no obvious signs of active star formation regions or significant dust lanes. The galaxy does not appear to be undergoing a major merger or experiencing substantial tidal disturbance, although subtle asymmetries cannot be ruled out based on this image alone. Overall, the object appears to be a relatively massive, quiescent galaxy at intermediate redshift.
