The galaxy appears to be a relatively smooth, elliptical-like system at a redshift of approximately 0.167. The central region exhibits a concentrated, bright yellowish hue, suggesting a population of older stars. The overall shape appears somewhat elongated. There are no distinct spiral arm structures or significant dust lanes visible in this image, indicating a potential lack of active star formation. A slight bluer color at the edges, compared to the central region, may suggest a small amount of ongoing star formation on the outskirts, or potentially the presence of a younger stellar population relative to the core. There is no sign of a major merger or significant tidal disturbances. However, a very slight irregularity in the overall shape may indicate a potential minor interaction with another galaxy at some point in the past. The galaxy exhibits a moderate mass.
