This galaxy presents as a relatively small, elongated system, likely an elliptical galaxy based on its overall shape and smooth appearance. The light distribution suggests a central concentration, with intensity gradually decreasing outwards. The galaxy appears to be cigar shaped with a slight asymmetry along its major axis. There is some indication of a possible minor disturbance or tidal feature, based on slight visual irregularities in the halo. The colors suggest there may be a mix of older stellar populations, with a redder hue more prevalent on one end. No distinct spiral arms or significant dust lanes are discernible. Overall, the galaxy appears as an early-type system showing signs of past gravitational interaction.
