The galaxy presents as an elliptical morphology. It exhibits a smooth, diffuse appearance with a concentrated central bulge. The light distribution suggests a relatively even stellar population throughout the galaxy, with no apparent spiral arms or dust lanes visible at this resolution. There is a slight elongation to its shape, indicating it may be an E4-E5 type elliptical, with a ratio of minor to major axis of approximately 0.6. The galaxy appears to have a yellowish-red hue, suggesting a population dominated by older, redder stars, indicative of a reduced rate of star formation. No signs of significant mergers or tidal disturbances are readily apparent. The galaxy appears relatively isolated, without obvious interactions with nearby companions.
