The galaxy presents an overall elongated, elliptical morphology. The central region exhibits a concentrated, bright core, suggesting a relatively high stellar density. This brightness diminishes gradually towards the edges, although the low image resolution obscures finer structural details. There appears to be a slight disk visible, observed nearly edge-on. There is little evidence of recent or ongoing major merger activity. The light distribution appears relatively smooth, hinting that the galaxy is likely an older system, although there may be ongoing star formation with a low rate. Based on color, the galaxy appears to contain a mix of stellar populations, with older, redder stars dominating the core and potentially bluer, younger stars contributing to the light from the outer regions.
