The galaxy presents as a moderately bright, compact object with a relatively smooth, elliptical morphology. It appears primarily spheroidal in shape, exhibiting minimal disk-like features. The central region is characterized by a concentrated luminosity, suggesting a dense stellar population or the presence of an active galactic nucleus (AGN). The overall color profile indicates a redder hue, possibly indicative of an older stellar population with reduced ongoing star formation. There is a very small hint of some distortion. The galaxy does not obviously appear to be undergoing any major merging activity or show signs of significant tidal disturbances.
