The galaxy presents a largely smooth morphology, appearing elliptical in shape, with an approximate physical radius of 7.8 kpc. The central region exhibits a bright, concentrated luminosity profile, suggesting a significant stellar population. There is a slight color gradient visible, transitioning from a warmer, yellower hue in the core to slightly cooler tones in the outer regions. The galaxy shows little evidence of distinct spiral arms or prominent dust lanes. The overall appearance indicates a relatively evolved system, possibly with a relatively low ongoing star formation rate. There appears to be little to no visible signs of any significant merger activity. The morphology seems more consistent with an elliptical galaxy exhibiting characteristics of a spheroid system dominated by older stellar populations.
